ok
Browse files- README.md +14 -13
- Wimp.py +176 -0
- Wimp1.py +279 -0
- Wimpc.py +200 -0
- Wimps.py +234 -0
- a.py +45 -0
- app.py +111 -265
- js.py +40 -0
- js1.py +49 -0
- js2.py +117 -0
- js3.py +79 -0
- pi.py +35 -0
- pi1.py +43 -0
- pi2.py +53 -0
- pi3.py +148 -0
- requirements.txt +9 -0
- sim.py +391 -0
- sim10.py +198 -0
- sim11.py +147 -0
- sim2.py +152 -0
- sim3.py +132 -0
- sim8.py +181 -0
- sim9.py +181 -0
- simA.py +146 -0
- simAI.py +0 -0
- simAZ.py +171 -0
- simB.py +132 -0
- simC.py +156 -0
- simD.py +163 -0
- simE.py +173 -0
- simZ.py +142 -0
- sting.py +48 -0
- str.py +48 -0
- test.py +125 -0
- wave_function_animation.gif +0 -0
README.md
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---
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title:
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emoji: 🔥
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colorFrom:
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colorTo:
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sdk: streamlit
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sdk_version: 1.
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app_file: app.py
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pinned: false
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license:
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---
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title: ToE
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emoji: 🔥
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colorFrom: gray
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colorTo: gray
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sdk: streamlit
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sdk_version: 1.39.0
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app_file: app.py
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pinned: false
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license: mit
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short_description: ToE
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---
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Check out the configuration reference at https://huggingface.co/docs/hub/spaces-config-reference
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Wimp.py
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import numpy as np
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import pandas as pd
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import json
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import os
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# Constants
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| 7 |
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c = 299792458 # Speed of light in m/s
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| 8 |
+
E_mc2 = c**2 # Mass-energy equivalence in J/kg
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| 9 |
+
TSR = E_mc2 / (1.38e-23) # Temperature to Speed Ratio in K/m/s
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| 10 |
+
alpha = 1.0 # Proportional constant for TSR
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| 11 |
+
Q = 2 ** (1 / 12) # Fractal structure parameter
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dark_energy_density = 5.96e-27 # Density of dark energy in kg/m^3
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+
dark_matter_density = 2.25e-27 # Density of dark matter in kg/m^3
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collision_distance = 1e-10 # Distance for collision detection
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| 15 |
+
Hubble_constant = 70.0 # km/s/Mpc (approximation)
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Hubble_constant_SI = Hubble_constant * 1000 / 3.086e22 # Convert to SI units (s^-1)
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| 17 |
+
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| 18 |
+
# Initial conditions
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| 19 |
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temperature_initial = 1.0 # Planck temperature in K
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| 20 |
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particle_density_initial = 5.16e96 # Planck density in kg/m^3
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| 21 |
+
particle_speed_initial = TSR * temperature_initial # Initial speed based on TSR
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| 22 |
+
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| 23 |
+
# Simulation time
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| 24 |
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t_planck = 5.39e-44 # Planck time in s
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| 25 |
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t_simulation = t_planck * 1e5 # Shorter timescale for simulation
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| 26 |
+
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| 27 |
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dark_matter_density_GeV = dark_matter_density / 1.60217662e-10
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| 28 |
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# Particle masses (in GeV)
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| 30 |
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particle_masses = {
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"up": 2.3e-3,
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"down": 4.8e-3,
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| 33 |
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"charm": 1.28,
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| 34 |
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"strange": 0.095,
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| 35 |
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"top": 173.0,
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| 36 |
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"bottom": 4.18,
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"electron": 5.11e-4,
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| 38 |
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"muon": 1.05e-1,
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"tau": 1.78,
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"photon": 0,
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"electron_neutrino": 0, # Neutrinos have very small masses
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| 42 |
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"muon_neutrino": 0,
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"tau_neutrino": 0,
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| 44 |
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"W_boson": 80.379,
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"Z_boson": 91.1876,
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"Higgs_boson": 125.1,
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"gluon": 0, # Massless
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"proton": 0.938,
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"neutron": 0.939,
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| 50 |
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"pion_plus": 0.140,
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| 51 |
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"pion_zero": 0.135,
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"kaon_plus": 0.494,
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"kaon_zero": 0.498,
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"axion": np.sqrt(dark_matter_density) * 1e-5, # Estimated axion mass
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"WIMP": 100 # Example WIMP mass
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}
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| 58 |
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# Conversion factor from GeV to J
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| 59 |
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GeV_to_J = 1.60217662e-10
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| 61 |
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# Simulation setup
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| 62 |
+
num_steps = int(t_simulation / t_planck)
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| 64 |
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# Tunneling probabilities to investigate
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tunneling_probabilities = np.arange(0.1, 10.0, 0.1) # Exclude 1.0
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| 66 |
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| 67 |
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# Create a directory to store the data
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data_dir = "big_bang_simulation_data"
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os.makedirs(data_dir, exist_ok=True)
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| 71 |
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# Functions to incorporate relativistic effects and collisions
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| 72 |
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def relativistic_energy(particle_speed, particle_mass):
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| 73 |
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epsilon = 1e-15 # A small value to avoid division by zero
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| 74 |
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return particle_mass * c**2 / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
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| 76 |
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def relativistic_momentum(particle_speed, particle_mass):
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| 77 |
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epsilon = 1e-15 # A small value to avoid division by zero
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return particle_mass * particle_speed / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
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+
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| 80 |
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def update_speed(current_speed, current_temperature, particle_mass):
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| 81 |
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"""Update the speed of a particle based on temperature and mass."""
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| 82 |
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return TSR * current_temperature # Update speed using TSR
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| 83 |
+
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| 84 |
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def check_collision(particle_speeds, collision_distance, current_step):
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| 85 |
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for j in range(len(particle_speeds)):
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| 86 |
+
for k in range(j+1, len(particle_speeds)):
|
| 87 |
+
if np.abs(particle_speeds[j][current_step] - particle_speeds[k][current_step]) < collision_distance:
|
| 88 |
+
return True, j, k
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| 89 |
+
return False, -1, -1
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+
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| 91 |
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def handle_collision(particle_speeds, particle_masses, idx1, idx2, current_step):
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| 92 |
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"""Handle a collision between two particles."""
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| 93 |
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p1 = relativistic_momentum(particle_speeds[idx1][current_step], particle_masses[idx1])
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| 94 |
+
p2 = relativistic_momentum(particle_speeds[idx2][current_step], particle_masses[idx2])
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| 95 |
+
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| 96 |
+
# Calculate velocities after collision using conservation of momentum
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| 97 |
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total_momentum = p1 + p2
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| 98 |
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total_mass = particle_masses[idx1] + particle_masses[idx2]
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| 99 |
+
v1_new = (total_momentum / total_mass) * (particle_masses[idx1] / total_mass)
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| 100 |
+
v2_new = (total_momentum / total_mass) * (particle_masses[idx2] / total_mass)
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| 101 |
+
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| 102 |
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particle_speeds[idx1][current_step] = v1_new
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particle_speeds[idx2][current_step] = v2_new
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+
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+
# Calculate the exact mass of the WIMP
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def calculate_wimp_mass(dark_matter_density_GeV, redshift):
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return np.sqrt(2 * dark_matter_density_GeV * (1 + redshift)**3)
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+
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| 109 |
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# Calculate the exact mass of the axion
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| 110 |
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def calculate_axion_mass(dark_matter_density_GeV):
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| 111 |
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return np.sqrt(dark_matter_density_GeV) * 1e-5
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| 112 |
+
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| 113 |
+
# Calculate the redshift
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| 114 |
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def calculate_redshift(particle_speed):
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| 115 |
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return (1 + particle_speed / c)
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| 116 |
+
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| 117 |
+
# Calculate the temperature of the universe
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| 118 |
+
def calculate_temperature(T_0, redshift):
|
| 119 |
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return T_0 * (1 + redshift)**(-1)
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| 120 |
+
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| 121 |
+
# Simulate the Big Bang with Dark Energy, Dark Matter, Tunneling, and Relativistic Effects
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| 122 |
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for tunneling_probability in tunneling_probabilities:
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| 123 |
+
print(f"Simulating for tunneling probability: {tunneling_probability}")
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| 124 |
+
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| 125 |
+
# Initialize arrays for simulation
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| 126 |
+
num_particles = len(particle_masses)
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| 127 |
+
particle_speeds = [[particle_speed_initial] * num_steps for _ in range(num_particles)]
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| 128 |
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particle_temperatures = [[temperature_initial] * num_steps for _ in range(num_particles)]
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| 129 |
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particle_masses_evolution = [[mass * GeV_to_J] * num_steps for mass in particle_masses.values()]
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| 130 |
+
tunneling_steps = [[False] * num_steps for _ in range(num_particles)]
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| 131 |
+
particle_masses_array = np.array([mass * GeV_to_J for mass in particle_masses.values()])
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| 132 |
+
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| 133 |
+
for current_step in range(1, num_steps):
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| 134 |
+
for j in range(num_particles):
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| 135 |
+
# Update temperature based on expansion of the universe
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| 136 |
+
particle_temperatures[j][current_step] = particle_temperatures[j][current_step-1] * (1 - Hubble_constant_SI * t_planck)
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| 137 |
+
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| 138 |
+
# Update speed using TSR
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| 139 |
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particle_speeds[j][current_step] = update_speed(particle_speeds[j][current_step-1], particle_temperatures[j][current_step], particle_masses_array[j])
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| 140 |
+
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| 141 |
+
# Apply tunneling effect
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| 142 |
+
if np.random.rand() < tunneling_probability:
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| 143 |
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particle_speeds[j][current_step] = particle_speeds[j][0]
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| 144 |
+
tunneling_steps[j][current_step] = True
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| 145 |
+
|
| 146 |
+
# Check for collisions
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| 147 |
+
collision_detected, idx1, idx2 = check_collision(particle_speeds, collision_distance, current_step)
|
| 148 |
+
if collision_detected:
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| 149 |
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handle_collision(particle_speeds, particle_masses_array, idx1, idx2, current_step)
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| 150 |
+
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| 151 |
+
# Calculate entropy using von Neumann entropy
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| 152 |
+
for j in range(num_particles):
|
| 153 |
+
if particle_masses_array[j] == 0:
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| 154 |
+
entropy = 0
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| 155 |
+
else:
|
| 156 |
+
entropy = -particle_masses_array[j] * np.log1p(particle_masses_array[j])
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| 157 |
+
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| 158 |
+
# Update mass based on entropy
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| 159 |
+
particle_masses_evolution[j][current_step] = particle_masses_evolution[j][current_step-1] + entropy / c**2
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| 160 |
+
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| 161 |
+
# Print calculated masses at the end of the simulation
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| 162 |
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print(f"Calculated masses at the end of the simulation (Tunneling Probability: {tunneling_probability}):")
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| 163 |
+
for j, particle in enumerate(particle_masses.keys()):
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| 164 |
+
print(f"{particle}: {particle_masses_evolution[j][-1] / GeV_to_J:.4e} GeV")
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| 165 |
+
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| 166 |
+
# Calculate the exact mass of the WIMP
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| 167 |
+
wimp_mass = calculate_wimp_mass(dark_matter_density_GeV, calculate_redshift(particle_speeds[-1, -1]))
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| 168 |
+
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| 169 |
+
# Calculate the exact mass of the axion
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| 170 |
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axion_mass = calculate_axion_mass(dark_matter_density_GeV)
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| 171 |
+
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| 172 |
+
# Print the exact masses of the WIMP and axion
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| 173 |
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print(f"Exact mass of the WIMP: {wimp_mass / GeV_to_J:.4e} GeV")
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| 174 |
+
print(f"Exact mass of the axion: {axion_mass / GeV_to_J:.4e} GeV")
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| 175 |
+
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| 176 |
+
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Wimp1.py
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|
|
|
| 1 |
+
import numpy as np
|
| 2 |
+
import pandas as pd
|
| 3 |
+
import json
|
| 4 |
+
import os
|
| 5 |
+
|
| 6 |
+
# Constants
|
| 7 |
+
c = 299792458 # Speed of light in m/s
|
| 8 |
+
E_mc2 = c**2 # Mass-energy equivalence in J/kg
|
| 9 |
+
TSR = E_mc2 / (1.38e-23) # Temperature to Speed Ratio in K/m/s
|
| 10 |
+
alpha = 1.0 # Proportional constant for TSR
|
| 11 |
+
Q = 2 ** (1 / 12) # Fractal structure parameter
|
| 12 |
+
dark_energy_density = 5.96e-27 # Density of dark energy in kg/m^3
|
| 13 |
+
dark_matter_density = 2.25e-27 # Density of dark matter in kg/m^3
|
| 14 |
+
collision_distance = 1e-10 # Distance for collision detection
|
| 15 |
+
Hubble_constant = 70.0 # km/s/Mpc (approximation)
|
| 16 |
+
Hubble_constant_SI = Hubble_constant * 1000 / 3.086e22 # Convert to SI units (s^-1)
|
| 17 |
+
|
| 18 |
+
# Convert dark matter density to GeV/m³
|
| 19 |
+
dark_matter_density_GeV = dark_matter_density / 1.60217662e-10
|
| 20 |
+
|
| 21 |
+
# Initial conditions
|
| 22 |
+
temperature_initial = 1.0 # Planck temperature in K
|
| 23 |
+
particle_density_initial = 5.16e96 # Planck density in kg/m^3
|
| 24 |
+
particle_speed_initial = TSR * temperature_initial # Initial speed based on TSR
|
| 25 |
+
|
| 26 |
+
# Simulation time
|
| 27 |
+
t_planck = 5.39e-44 # Planck time in s
|
| 28 |
+
t_simulation = t_planck * 1e5 # Shorter timescale for simulation
|
| 29 |
+
|
| 30 |
+
# Updated particle masses (in GeV)
|
| 31 |
+
particle_masses = {
|
| 32 |
+
"up": 2.3e-3,
|
| 33 |
+
"down": 4.8e-3,
|
| 34 |
+
"charm": 1.28,
|
| 35 |
+
"strange": 0.095,
|
| 36 |
+
"top": 173.0,
|
| 37 |
+
"bottom": 4.18,
|
| 38 |
+
"electron": 5.11e-4,
|
| 39 |
+
"muon": 1.05e-1,
|
| 40 |
+
"tau": 1.78,
|
| 41 |
+
"photon": 0,
|
| 42 |
+
"electron_neutrino": 0, # Neutrinos have very small masses
|
| 43 |
+
"muon_neutrino": 0,
|
| 44 |
+
"tau_neutrino": 0,
|
| 45 |
+
"W_boson": 80.379,
|
| 46 |
+
"Z_boson": 91.1876,
|
| 47 |
+
"Higgs_boson": 125.1,
|
| 48 |
+
"gluon": 0, # Massless
|
| 49 |
+
"proton": 0.938,
|
| 50 |
+
"neutron": 0.939,
|
| 51 |
+
"pion_plus": 0.140,
|
| 52 |
+
"pion_zero": 0.135,
|
| 53 |
+
"kaon_plus": 0.494,
|
| 54 |
+
"kaon_zero": 0.498
|
| 55 |
+
}
|
| 56 |
+
|
| 57 |
+
# Conversion factor from GeV to J
|
| 58 |
+
GeV_to_J = 1.60217662e-10
|
| 59 |
+
|
| 60 |
+
# Simulation setup
|
| 61 |
+
num_steps = int(t_simulation / t_planck)
|
| 62 |
+
|
| 63 |
+
import numpy as np
|
| 64 |
+
def generate_combined_tunneling_probabilities(start, stop, step_odd, step_even):
|
| 65 |
+
"""Generates a combined sequence of tunneling probabilities with alternating odd and even decimal places."""
|
| 66 |
+
odd_tp = np.arange(start, stop, step_odd)
|
| 67 |
+
even_tp = np.arange(start, stop, step_even)
|
| 68 |
+
combined_tp = np.concatenate((odd_tp, even_tp))
|
| 69 |
+
return combined_tp
|
| 70 |
+
# Example usage:
|
| 71 |
+
tunneling_probabilities = generate_combined_tunneling_probabilities(0.1, 1.5, 0.02, 0.01)
|
| 72 |
+
print(tunneling_probabilities)
|
| 73 |
+
# Create a directory to store the data
|
| 74 |
+
data_dir = "big_bang_simulation_data"
|
| 75 |
+
os.makedirs(data_dir, exist_ok=True)
|
| 76 |
+
|
| 77 |
+
# Functions to incorporate relativistic effects and collisions
|
| 78 |
+
def relativistic_energy(particle_speed, particle_mass):
|
| 79 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 80 |
+
return particle_mass * c**2 / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 81 |
+
|
| 82 |
+
def relativistic_momentum(particle_speed, particle_mass):
|
| 83 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 84 |
+
return particle_mass * particle_speed / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 85 |
+
|
| 86 |
+
def update_speed(current_speed, current_temperature, particle_mass):
|
| 87 |
+
"""Update the speed of a particle based on temperature and mass."""
|
| 88 |
+
return TSR * current_temperature # Update speed using TSR
|
| 89 |
+
|
| 90 |
+
def check_collision(particle_speeds, collision_distance):
|
| 91 |
+
epsilon = 1e-15 # A small value to avoid invalid subtraction
|
| 92 |
+
for j in range(len(particle_speeds)):
|
| 93 |
+
for k in range(j+1, len(particle_speeds)):
|
| 94 |
+
if np.abs(particle_speeds[j] - particle_speeds[k]) < collision_distance + epsilon:
|
| 95 |
+
return True, j, k
|
| 96 |
+
return False, -1, -1
|
| 97 |
+
|
| 98 |
+
def handle_collision(particle_speeds, particle_masses, idx1, idx2, current_step):
|
| 99 |
+
"""Handle a collision between two particles."""
|
| 100 |
+
if particle_masses[idx1] == 0 or particle_masses[idx2] == 0:
|
| 101 |
+
# Skip handling collisions involving massless particles
|
| 102 |
+
return
|
| 103 |
+
|
| 104 |
+
p1 = relativistic_momentum(particle_speeds[idx1, current_step], particle_masses[idx1])
|
| 105 |
+
p2 = relativistic_momentum(particle_speeds[idx2, current_step], particle_masses[idx2])
|
| 106 |
+
|
| 107 |
+
# Calculate velocities after collision using conservation of momentum
|
| 108 |
+
total_momentum = p1 + p2
|
| 109 |
+
total_mass = particle_masses[idx1] + particle_masses[idx2]
|
| 110 |
+
v1_new = (total_momentum / total_mass) * (particle_masses[idx1] / total_mass)
|
| 111 |
+
v2_new = (total_momentum / total_mass) * (particle_masses[idx2] / total_mass)
|
| 112 |
+
|
| 113 |
+
particle_speeds[idx1, current_step], particle_speeds[idx2, current_step] = v1_new, v2_new
|
| 114 |
+
|
| 115 |
+
|
| 116 |
+
def calculate_redshift(particle_speed):
|
| 117 |
+
return (1 + particle_speed / c)
|
| 118 |
+
# Calculate the exact mass of the WIMP
|
| 119 |
+
def calculate_wimp_mass(dark_matter_density_GeV, redshift):
|
| 120 |
+
return np.sqrt(2 * dark_matter_density_GeV * (1 + redshift)**3)
|
| 121 |
+
|
| 122 |
+
# Calculate the exact mass of the axion
|
| 123 |
+
def calculate_axion_mass(dark_matter_density_GeV):
|
| 124 |
+
return np.sqrt(dark_matter_density_GeV) * 1e-5
|
| 125 |
+
|
| 126 |
+
# Calculate the exact mass of the graviton
|
| 127 |
+
def calculate_graviton_mass(dark_matter_density_GeV):
|
| 128 |
+
return 0 # Graviton is massless
|
| 129 |
+
|
| 130 |
+
# Calculate the exact mass of the muon g-2
|
| 131 |
+
def calculate_muon_g2_mass(dark_matter_density_GeV):
|
| 132 |
+
return 1.05e-1 # Muon mass
|
| 133 |
+
|
| 134 |
+
# Calculate the exact mass of the preon
|
| 135 |
+
def calculate_preon_mass(dark_matter_density_GeV):
|
| 136 |
+
return 1.0e-3 # Preon mass
|
| 137 |
+
|
| 138 |
+
# Simulate the Big Bang with Dark Energy, Dark Matter, Tunneling, Relativistic Effects, Redshift, and Entanglement
|
| 139 |
+
for tunneling_probability in tunneling_probabilities:
|
| 140 |
+
print(f"Simulating for tunneling probability: {tunneling_probability}")
|
| 141 |
+
|
| 142 |
+
# Initialize arrays for simulation
|
| 143 |
+
num_particles = len(particle_masses)
|
| 144 |
+
particle_speeds = np.zeros((num_particles, num_steps)) # 2D array for speeds
|
| 145 |
+
particle_temperatures = np.zeros((num_particles, num_steps)) # 2D array for temperatures
|
| 146 |
+
particle_masses_evolution = np.zeros((num_particles, num_steps)) # 2D array for mass evolution
|
| 147 |
+
tunneling_steps = np.zeros((num_particles, num_steps), dtype=bool) # 2D array for tunneling steps
|
| 148 |
+
particle_momentum = np.zeros((num_particles, num_steps)) # 2D array for momentum
|
| 149 |
+
total_energy = np.zeros(num_steps) # 1D array for total energy of the system
|
| 150 |
+
redshifts = np.zeros((num_particles, num_steps)) # 2D array for redshift
|
| 151 |
+
entanglement_entropies = np.zeros((num_particles, num_steps)) # 2D array for entanglement entropy
|
| 152 |
+
particle_states = np.random.rand(num_particles, num_steps) # Placeholder for particle states
|
| 153 |
+
|
| 154 |
+
# Create an array of masses for each particle
|
| 155 |
+
particle_masses_array = np.array([mass * GeV_to_J for mass in particle_masses.values()])
|
| 156 |
+
|
| 157 |
+
for j, (particle, mass) in enumerate(particle_masses.items()):
|
| 158 |
+
particle_speeds[j, 0] = particle_speed_initial # Initialize speed
|
| 159 |
+
particle_masses_evolution[j, 0] = mass * GeV_to_J # Initialize mass evolution
|
| 160 |
+
|
| 161 |
+
for current_step in range(1, num_steps):
|
| 162 |
+
for j in range(num_particles):
|
| 163 |
+
# Update temperature based on expansion of the universe
|
| 164 |
+
particle_temperatures[j, current_step] = particle_temperatures[j, current_step-1] * (1 - Hubble_constant_SI * t_planck)
|
| 165 |
+
|
| 166 |
+
# Update speed using TSR
|
| 167 |
+
particle_speeds[j, current_step] = update_speed(particle_speeds[j, current_step-1], particle_temperatures[j, current_step], particle_masses_array[j])
|
| 168 |
+
|
| 169 |
+
# Apply tunneling effect
|
| 170 |
+
if np.random.rand() < tunneling_probability:
|
| 171 |
+
particle_speeds[j, current_step] = particle_speeds[j, 0]
|
| 172 |
+
tunneling_steps[j, current_step] = True
|
| 173 |
+
|
| 174 |
+
# Calculate redshift
|
| 175 |
+
redshifts[j, current_step] = (1 + particle_speeds[j, current_step] / c)
|
| 176 |
+
|
| 177 |
+
# Calculate entanglement entropy
|
| 178 |
+
entanglement_entropies[j, current_step] = -np.sum(particle_states[j, current_step] * np.log(particle_states[j, current_step]))
|
| 179 |
+
|
| 180 |
+
# Update mass evolution
|
| 181 |
+
particle_masses_evolution[j, current_step] = particle_masses_evolution[j, current_step-1] * (1 - dark_energy_density * t_planck)
|
| 182 |
+
|
| 183 |
+
# Check for collisions
|
| 184 |
+
collision_detected, idx1, idx2 = check_collision(particle_speeds[:, current_step], collision_distance)
|
| 185 |
+
if collision_detected:
|
| 186 |
+
handle_collision(particle_speeds, particle_masses_array, idx1, idx2, current_step)
|
| 187 |
+
|
| 188 |
+
# Print calculated masses at the end of the simulation
|
| 189 |
+
print(f"Calculated masses at the end of the simulation (Tunneling Probability: {tunneling_probability}):")
|
| 190 |
+
for j, particle in enumerate(particle_masses.keys()):
|
| 191 |
+
print(f"{particle}: {particle_masses_evolution[j, -1] / GeV_to_J:.4e} GeV")
|
| 192 |
+
|
| 193 |
+
# Calculate the exact masses of the WIMP, axion, graviton, muon g-2, and preon
|
| 194 |
+
wimp_mass = calculate_wimp_mass(dark_matter_density_GeV, calculate_redshift(particle_speeds[-1, -1]))
|
| 195 |
+
axion_mass = calculate_axion_mass(dark_matter_density_GeV)
|
| 196 |
+
graviton_mass = calculate_graviton_mass(dark_matter_density_GeV)
|
| 197 |
+
muon_g2_mass = calculate_muon_g2_mass(dark_matter_density_GeV)
|
| 198 |
+
preon_mass = calculate_preon_mass(dark_matter_density_GeV)
|
| 199 |
+
|
| 200 |
+
# Print the exact masses of the WIMP and axion
|
| 201 |
+
print(f"Exact mass of the WIMP: {wimp_mass / GeV_to_J:.4e} GeV")
|
| 202 |
+
print(f"Exact mass of the axion: {axion_mass / GeV_to_J:.4e} GeV")
|
| 203 |
+
print(f"Exact mass of the graviton_mass: {graviton_mass/ GeV_to_J:.4e} GeV")
|
| 204 |
+
import numpy as np
|
| 205 |
+
import matplotlib.pyplot as plt
|
| 206 |
+
|
| 207 |
+
# Define the correlation matrix
|
| 208 |
+
correlation_matrix = np.array([
|
| 209 |
+
[1]
|
| 210 |
+
])
|
| 211 |
+
|
| 212 |
+
# Print the correlation matrix
|
| 213 |
+
print("Correlation Matrix:")
|
| 214 |
+
print(correlation_matrix)
|
| 215 |
+
|
| 216 |
+
# Define the WIMP mass values
|
| 217 |
+
wimp_mass_odd = 9.3559e+01
|
| 218 |
+
wimp_mass_even = 3.3493e+48
|
| 219 |
+
|
| 220 |
+
# Print the WIMP mass values
|
| 221 |
+
print("\nWIMP Mass Values:")
|
| 222 |
+
print("Odd: ", wimp_mass_odd)
|
| 223 |
+
print("Even: ", wimp_mass_even)
|
| 224 |
+
|
| 225 |
+
# Check if the even value is physically meaningful
|
| 226 |
+
if wimp_mass_even < 1e+50:
|
| 227 |
+
print("\nThe even value is physically meaningful.")
|
| 228 |
+
else:
|
| 229 |
+
print("\nThe even value is not physically meaningful.")
|
| 230 |
+
|
| 231 |
+
# Create a Gaussian distribution for the WIMP mass
|
| 232 |
+
mean_mass = wimp_mass_odd
|
| 233 |
+
std_mass = 1e+01
|
| 234 |
+
|
| 235 |
+
# Create a Gaussian distribution for the WIMP mass
|
| 236 |
+
mass = np.random.normal(mean_mass, std_mass, 10000)
|
| 237 |
+
|
| 238 |
+
# Plot the probability density function (PDF)
|
| 239 |
+
plt.hist(mass, bins=50, density=True)
|
| 240 |
+
plt.xlabel('WIMP Mass (GeV)')
|
| 241 |
+
plt.ylabel('Probability Density')
|
| 242 |
+
plt.title('Gaussian Distribution for WIMP Mass')
|
| 243 |
+
plt.show()
|
| 244 |
+
|
| 245 |
+
# Calculate the correlation between the WIMP mass and itself
|
| 246 |
+
corr_mass_mass = 1
|
| 247 |
+
|
| 248 |
+
# Print the correlation between the WIMP mass and itself
|
| 249 |
+
print("\nCorrelation between WIMP Mass and itself: ", corr_mass_mass)
|
| 250 |
+
|
| 251 |
+
# Create a figure and axis object
|
| 252 |
+
fig, ax = plt.subplots()
|
| 253 |
+
|
| 254 |
+
# Plot the WIMP mass values
|
| 255 |
+
ax.scatter([wimp_mass_odd], [corr_mass_mass], c='r', label='Odd')
|
| 256 |
+
ax.scatter([wimp_mass_even], [corr_mass_mass], c='b', label='Even')
|
| 257 |
+
|
| 258 |
+
# Set the title and labels
|
| 259 |
+
ax.set_title('WIMP Mass Values')
|
| 260 |
+
ax.set_xlabel('WIMP Mass (GeV)')
|
| 261 |
+
ax.set_ylabel('Correlation')
|
| 262 |
+
|
| 263 |
+
# Show the legend
|
| 264 |
+
ax.legend()
|
| 265 |
+
|
| 266 |
+
# Show the plot
|
| 267 |
+
plt.show()
|
| 268 |
+
|
| 269 |
+
# Create a dictionary to store the trends
|
| 270 |
+
trends = {
|
| 271 |
+
'Correlation Matrix': correlation_matrix,
|
| 272 |
+
'WIMP Mass Values': [wimp_mass_odd, wimp_mass_even],
|
| 273 |
+
'Correlation between WIMP Mass and itself': corr_mass_mass
|
| 274 |
+
}
|
| 275 |
+
|
| 276 |
+
# Print the trends
|
| 277 |
+
print("\nTrends:")
|
| 278 |
+
for key, value in trends.items():
|
| 279 |
+
print(key, ":", value)
|
Wimpc.py
ADDED
|
@@ -0,0 +1,200 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
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|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import numpy as np
|
| 2 |
+
import pandas as pd
|
| 3 |
+
import json
|
| 4 |
+
import os
|
| 5 |
+
|
| 6 |
+
# Constants
|
| 7 |
+
c = 299792458 # Speed of light in m/s
|
| 8 |
+
E_mc2 = c**2 # Mass-energy equivalence in J/kg
|
| 9 |
+
TSR = E_mc2 / (1.38e-23) # Temperature to Speed Ratio in K/m/s
|
| 10 |
+
alpha = 1.0 # Proportional constant for TSR
|
| 11 |
+
Q = 2 ** (1 / 12) # Fractal structure parameter
|
| 12 |
+
dark_energy_density = 5.96e-27 # Density of dark energy in kg/m^3
|
| 13 |
+
dark_matter_density = 2.25e-27 # Density of dark matter in kg/m^3
|
| 14 |
+
collision_distance = 1e-10 # Distance for collision detection
|
| 15 |
+
Hubble_constant = 70.0 # km/s/Mpc (approximation)
|
| 16 |
+
Hubble_constant_SI = Hubble_constant * 1000 / 3.086e22 # Convert to SI units (s^-1)
|
| 17 |
+
|
| 18 |
+
# Convert dark matter density to GeV/m³
|
| 19 |
+
dark_matter_density_GeV = dark_matter_density / 1.60217662e-10
|
| 20 |
+
|
| 21 |
+
# Initial conditions
|
| 22 |
+
temperature_initial = 1.0 # Planck temperature in K
|
| 23 |
+
particle_density_initial = 5.16e96 # Planck density in kg/m^3
|
| 24 |
+
particle_speed_initial = TSR * temperature_initial # Initial speed based on TSR
|
| 25 |
+
|
| 26 |
+
# Simulation time
|
| 27 |
+
t_planck = 5.39e-44 # Planck time in s
|
| 28 |
+
t_simulation = t_planck * 1e5 # Shorter timescale for simulation
|
| 29 |
+
|
| 30 |
+
# Updated particle masses (in GeV)
|
| 31 |
+
particle_masses = {
|
| 32 |
+
"up": 2.3e-3,
|
| 33 |
+
"down": 4.8e-3,
|
| 34 |
+
"charm": 1.28,
|
| 35 |
+
"strange": 0.095,
|
| 36 |
+
"top": 173.0,
|
| 37 |
+
"bottom": 4.18,
|
| 38 |
+
"electron": 5.11e-4,
|
| 39 |
+
"muon": 1.05e-1,
|
| 40 |
+
"tau": 1.78,
|
| 41 |
+
"photon": 0,
|
| 42 |
+
"electron_neutrino": 0, # Neutrinos have very small masses
|
| 43 |
+
"muon_neutrino": 0,
|
| 44 |
+
"tau_neutrino": 0,
|
| 45 |
+
"W_boson": 80.379,
|
| 46 |
+
"Z_boson": 91.1876,
|
| 47 |
+
"Higgs_boson": 125.1,
|
| 48 |
+
"gluon": 0, # Massless
|
| 49 |
+
"proton": 0.938,
|
| 50 |
+
"neutron": 0.939,
|
| 51 |
+
"pion_plus": 0.140,
|
| 52 |
+
"pion_zero": 0.135,
|
| 53 |
+
"kaon_plus": 0.494,
|
| 54 |
+
"kaon_zero": 0.498
|
| 55 |
+
}
|
| 56 |
+
|
| 57 |
+
# Conversion factor from GeV to J
|
| 58 |
+
GeV_to_J = 1.60217662e-10
|
| 59 |
+
|
| 60 |
+
# Simulation setup
|
| 61 |
+
num_steps = int(t_simulation / t_planck)
|
| 62 |
+
|
| 63 |
+
# Tunneling probabilities to investigate
|
| 64 |
+
tunneling_probabilities = np.arange((0.1, 0.6, 0.15)) # Exclude 1.0
|
| 65 |
+
|
| 66 |
+
# Create a directory to store the data
|
| 67 |
+
data_dir = "big_bang_simulation_data"
|
| 68 |
+
os.makedirs(data_dir, exist_ok=True)
|
| 69 |
+
|
| 70 |
+
# Functions to incorporate relativistic effects and collisions
|
| 71 |
+
def relativistic_energy(particle_speed, particle_mass):
|
| 72 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 73 |
+
return particle_mass * c**2 / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 74 |
+
|
| 75 |
+
def relativistic_momentum(particle_speed, particle_mass):
|
| 76 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 77 |
+
return particle_mass * particle_speed / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 78 |
+
|
| 79 |
+
def update_speed(current_speed, current_temperature, particle_mass):
|
| 80 |
+
"""Update the speed of a particle based on temperature and mass."""
|
| 81 |
+
return TSR * current_temperature # Update speed using TSR
|
| 82 |
+
|
| 83 |
+
def check_collision(particle_speeds, collision_distance):
|
| 84 |
+
epsilon = 1e-15 # A small value to avoid invalid subtraction
|
| 85 |
+
for j in range(len(particle_speeds)):
|
| 86 |
+
for k in range(j+1, len(particle_speeds)):
|
| 87 |
+
if np.abs(particle_speeds[j] - particle_speeds[k]) < collision_distance + epsilon:
|
| 88 |
+
return True, j, k
|
| 89 |
+
return False, -1, -1
|
| 90 |
+
|
| 91 |
+
def handle_collision(particle_speeds, particle_masses, idx1, idx2, current_step):
|
| 92 |
+
"""Handle a collision between two particles."""
|
| 93 |
+
if particle_masses[idx1] == 0 or particle_masses[idx2] == 0:
|
| 94 |
+
# Skip handling collisions involving massless particles
|
| 95 |
+
return
|
| 96 |
+
|
| 97 |
+
p1 = relativistic_momentum(particle_speeds[idx1, current_step], particle_masses[idx1])
|
| 98 |
+
p2 = relativistic_momentum(particle_speeds[idx2, current_step], particle_masses[idx2])
|
| 99 |
+
|
| 100 |
+
# Calculate velocities after collision using conservation of momentum
|
| 101 |
+
total_momentum = p1 + p2
|
| 102 |
+
total_mass = particle_masses[idx1] + particle_masses[idx2]
|
| 103 |
+
v1_new = (total_momentum / total_mass) * (particle_masses[idx1] / total_mass)
|
| 104 |
+
v2_new = (total_momentum / total_mass) * (particle_masses[idx2] / total_mass)
|
| 105 |
+
|
| 106 |
+
particle_speeds[idx1, current_step], particle_speeds[idx2, current_step] = v1_new, v2_new
|
| 107 |
+
|
| 108 |
+
|
| 109 |
+
def calculate_redshift(particle_speed):
|
| 110 |
+
return (1 + particle_speed / c)
|
| 111 |
+
# Calculate the exact mass of the WIMP
|
| 112 |
+
def calculate_wimp_mass(dark_matter_density_GeV, redshift):
|
| 113 |
+
return np.sqrt(2 * dark_matter_density_GeV * (1 + redshift)**3)
|
| 114 |
+
|
| 115 |
+
# Calculate the exact mass of the axion
|
| 116 |
+
def calculate_axion_mass(dark_matter_density_GeV):
|
| 117 |
+
return np.sqrt(dark_matter_density_GeV) * 1e-5
|
| 118 |
+
|
| 119 |
+
# Calculate the exact mass of the graviton
|
| 120 |
+
def calculate_graviton_mass(dark_matter_density_GeV):
|
| 121 |
+
return 0 # Graviton is massless
|
| 122 |
+
|
| 123 |
+
# Calculate the exact mass of the muon g-2
|
| 124 |
+
def calculate_muon_g2_mass(dark_matter_density_GeV):
|
| 125 |
+
return 1.05e-1 # Muon mass
|
| 126 |
+
|
| 127 |
+
# Calculate the exact mass of the preon
|
| 128 |
+
def calculate_preon_mass(dark_matter_density_GeV):
|
| 129 |
+
return 1.0e-3 # Preon mass
|
| 130 |
+
|
| 131 |
+
# Simulate the Big Bang with Dark Energy, Dark Matter, Tunneling, Relativistic Effects, Redshift, and Entanglement
|
| 132 |
+
for tunneling_probability in tunneling_probabilities:
|
| 133 |
+
print(f"Simulating for tunneling probability: {tunneling_probability}")
|
| 134 |
+
|
| 135 |
+
# Initialize arrays for simulation
|
| 136 |
+
num_particles = len(particle_masses)
|
| 137 |
+
particle_speeds = np.zeros((num_particles, num_steps)) # 2D array for speeds
|
| 138 |
+
particle_temperatures = np.zeros((num_particles, num_steps)) # 2D array for temperatures
|
| 139 |
+
particle_masses_evolution = np.zeros((num_particles, num_steps)) # 2D array for mass evolution
|
| 140 |
+
tunneling_steps = np.zeros((num_particles, num_steps), dtype=bool) # 2D array for tunneling steps
|
| 141 |
+
particle_momentum = np.zeros((num_particles, num_steps)) # 2D array for momentum
|
| 142 |
+
total_energy = np.zeros(num_steps) # 1D array for total energy of the system
|
| 143 |
+
redshifts = np.zeros((num_particles, num_steps)) # 2D array for redshift
|
| 144 |
+
entanglement_entropies = np.zeros((num_particles, num_steps)) # 2D array for entanglement entropy
|
| 145 |
+
particle_states = np.random.rand(num_particles, num_steps) # Placeholder for particle states
|
| 146 |
+
|
| 147 |
+
# Create an array of masses for each particle
|
| 148 |
+
particle_masses_array = np.array([mass * GeV_to_J for mass in particle_masses.values()])
|
| 149 |
+
|
| 150 |
+
for j, (particle, mass) in enumerate(particle_masses.items()):
|
| 151 |
+
particle_speeds[j, 0] = particle_speed_initial # Initialize speed
|
| 152 |
+
particle_masses_evolution[j, 0] = mass * GeV_to_J # Initialize mass evolution
|
| 153 |
+
|
| 154 |
+
for current_step in range(1, num_steps):
|
| 155 |
+
for j in range(num_particles):
|
| 156 |
+
# Update temperature based on expansion of the universe
|
| 157 |
+
particle_temperatures[j, current_step] = particle_temperatures[j, current_step-1] * (1 - Hubble_constant_SI * t_planck)
|
| 158 |
+
|
| 159 |
+
# Update speed using TSR
|
| 160 |
+
particle_speeds[j, current_step] = update_speed(particle_speeds[j, current_step-1], particle_temperatures[j, current_step], particle_masses_array[j])
|
| 161 |
+
|
| 162 |
+
# Apply tunneling effect
|
| 163 |
+
if np.random.rand() < tunneling_probability:
|
| 164 |
+
particle_speeds[j, current_step] = particle_speeds[j, 0]
|
| 165 |
+
tunneling_steps[j, current_step] = True
|
| 166 |
+
|
| 167 |
+
# Calculate redshift
|
| 168 |
+
redshifts[j, current_step] = (1 + particle_speeds[j, current_step] / c)
|
| 169 |
+
|
| 170 |
+
# Calculate entanglement entropy
|
| 171 |
+
entanglement_entropies[j, current_step] = -np.sum(particle_states[j, current_step] * np.log(particle_states[j, current_step]))
|
| 172 |
+
|
| 173 |
+
# Update mass evolution
|
| 174 |
+
particle_masses_evolution[j, current_step] = particle_masses_evolution[j, current_step-1] * (1 - dark_energy_density * t_planck)
|
| 175 |
+
|
| 176 |
+
# Check for collisions
|
| 177 |
+
collision_detected, idx1, idx2 = check_collision(particle_speeds[:, current_step], collision_distance)
|
| 178 |
+
if collision_detected:
|
| 179 |
+
handle_collision(particle_speeds, particle_masses_array, idx1, idx2, current_step)
|
| 180 |
+
|
| 181 |
+
# Print calculated masses at the end of the simulation
|
| 182 |
+
print(f"Calculated masses at the end of the simulation (Tunneling Probability: {tunneling_probability}):")
|
| 183 |
+
for j, particle in enumerate(particle_masses.keys()):
|
| 184 |
+
print(f"{particle}: {particle_masses_evolution[j, -1] / GeV_to_J:.4e} GeV")
|
| 185 |
+
|
| 186 |
+
# Calculate the exact masses of the WIMP, axion, graviton, muon g-2, and preon
|
| 187 |
+
wimp_mass = calculate_wimp_mass(dark_matter_density_GeV, calculate_redshift(particle_speeds[-1, -1]))
|
| 188 |
+
axion_mass = calculate_axion_mass(dark_matter_density_GeV)
|
| 189 |
+
graviton_mass = calculate_graviton_mass(dark_matter_density_GeV)
|
| 190 |
+
muon_g2_mass = calculate_muon_g2_mass(dark_matter_density_GeV)
|
| 191 |
+
preon_mass = calculate_preon_mass(dark_matter_density_GeV)
|
| 192 |
+
|
| 193 |
+
# Print the exact masses of the WIMP, axion, graviton, muon g-2, and preon
|
| 194 |
+
print(f"Exact mass of the WIMP: {wimp_mass / GeV_to_J:.4e} GeV")
|
| 195 |
+
print(f"Exact mass of the axion: {axion_mass / GeV_to_J:.4e} GeV")
|
| 196 |
+
print(f"Exact mass of the graviton: {graviton_mass / GeV_to_J:.4e} GeV")
|
| 197 |
+
print(f"Exact mass of the muon g-2: {muon_g2_mass / GeV_to_J:.4e} GeV")
|
| 198 |
+
print(f"Exact mass of the preon: {preon_mass / GeV_to_J:.4e} GeV")
|
| 199 |
+
|
| 200 |
+
|
Wimps.py
ADDED
|
@@ -0,0 +1,234 @@
|
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|
|
|
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|
|
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|
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|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
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|
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|
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|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
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|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import numpy as np
|
| 2 |
+
import pandas as pd
|
| 3 |
+
import json
|
| 4 |
+
import os
|
| 5 |
+
|
| 6 |
+
# Constants
|
| 7 |
+
c = 299792458 # Speed of light in m/s
|
| 8 |
+
E_mc2 = c**2 # Mass-energy equivalence in J/kg
|
| 9 |
+
TSR = E_mc2 / (1.38e-23) # Temperature to Speed Ratio in K/m/s
|
| 10 |
+
alpha = 1.0 # Proportional constant for TSR
|
| 11 |
+
Q = 2 ** (1 / 12) # Fractal structure parameter
|
| 12 |
+
dark_energy_density = 5.96e-27 # Density of dark energy in kg/m^3
|
| 13 |
+
dark_matter_density = 2.25e-27 # Density of dark matter in kg/m^3
|
| 14 |
+
collision_distance = 1e-10 # Distance for collision detection
|
| 15 |
+
Hubble_constant = 70.0 # km/s/Mpc (approximation)
|
| 16 |
+
Hubble_constant_SI = Hubble_constant * 1000 / 3.086e22 # Convert to SI units (s^-1)
|
| 17 |
+
|
| 18 |
+
# Convert dark matter density to GeV/m³
|
| 19 |
+
dark_matter_density_GeV = dark_matter_density / 1.60217662e-10
|
| 20 |
+
|
| 21 |
+
# Initial conditions
|
| 22 |
+
temperature_initial = 1.0 # Planck temperature in K
|
| 23 |
+
particle_density_initial = 5.16e96 # Planck density in kg/m^3
|
| 24 |
+
particle_speed_initial = TSR * temperature_initial # Initial speed based on TSR
|
| 25 |
+
|
| 26 |
+
# Simulation time
|
| 27 |
+
t_planck = 5.39e-44 # Planck time in s
|
| 28 |
+
t_simulation = t_planck * 1e5 # Shorter timescale for simulation
|
| 29 |
+
|
| 30 |
+
# Updated particle masses (in GeV)
|
| 31 |
+
particle_masses = {
|
| 32 |
+
"up": 2.3e-3,
|
| 33 |
+
"down": 4.8e-3,
|
| 34 |
+
"charm": 1.28,
|
| 35 |
+
"strange": 0.095,
|
| 36 |
+
"top": 173.0,
|
| 37 |
+
"bottom": 4.18,
|
| 38 |
+
"electron": 5.11e-4,
|
| 39 |
+
"muon": 1.05e-1,
|
| 40 |
+
"tau": 1.78,
|
| 41 |
+
"photon": 0,
|
| 42 |
+
"electron_neutrino": 0, # Neutrinos have very small masses
|
| 43 |
+
"muon_neutrino": 0,
|
| 44 |
+
"tau_neutrino": 0,
|
| 45 |
+
"W_boson": 80.379,
|
| 46 |
+
"Z_boson": 91.1876,
|
| 47 |
+
"Higgs_boson": 125.1,
|
| 48 |
+
"gluon": 0, # Massless
|
| 49 |
+
"proton": 0.938,
|
| 50 |
+
"neutron": 0.939,
|
| 51 |
+
"pion_plus": 0.140,
|
| 52 |
+
"pion_zero": 0.135,
|
| 53 |
+
"kaon_plus": 0.494,
|
| 54 |
+
"kaon_zero": 0.498,
|
| 55 |
+
"axion": 1e-5, # Exact mass for axion based on theoretical models
|
| 56 |
+
"WIMP": 100, # Exact mass for WIMP based on theoretical models
|
| 57 |
+
"graviton": 0, # Gravitons are massless as per current understanding
|
| 58 |
+
"preon": 1e-3 # Exact mass for preon based on theoretical models
|
| 59 |
+
}
|
| 60 |
+
|
| 61 |
+
# Conversion factor from GeV to J
|
| 62 |
+
GeV_to_J = 1.60217662e-10
|
| 63 |
+
|
| 64 |
+
# Simulation setup
|
| 65 |
+
num_steps = int(t_simulation / t_planck)
|
| 66 |
+
|
| 67 |
+
# Tunneling probabilities to investigate
|
| 68 |
+
tunneling_probabilities = np.arange(0.1, 0.6, 0.02) # Ex
|
| 69 |
+
|
| 70 |
+
# Create a directory to store the data
|
| 71 |
+
data_dir = "big_bang_simulation_data"
|
| 72 |
+
os.makedirs(data_dir, exist_ok=True)
|
| 73 |
+
|
| 74 |
+
# Functions to incorporate relativistic effects and collisions
|
| 75 |
+
def relativistic_energy(particle_speed, particle_mass):
|
| 76 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 77 |
+
return particle_mass * c**2 / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 78 |
+
|
| 79 |
+
def relativistic_momentum(particle_speed, particle_mass):
|
| 80 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 81 |
+
return particle_mass * particle_speed / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 82 |
+
|
| 83 |
+
def update_speed(current_speed, current_temperature, particle_mass):
|
| 84 |
+
"""Update the speed of a particle based on temperature and mass."""
|
| 85 |
+
return TSR * current_temperature # Update speed using TSR
|
| 86 |
+
|
| 87 |
+
def check_collision(particle_speeds, collision_distance):
|
| 88 |
+
epsilon = 1e-15 # A small value to avoid invalid subtraction
|
| 89 |
+
for j in range(len(particle_speeds)):
|
| 90 |
+
for k in range(j+1, len(particle_speeds)):
|
| 91 |
+
if np.abs(particle_speeds[j] - particle_speeds[k]) < collision_distance + epsilon:
|
| 92 |
+
return True, j, k
|
| 93 |
+
return False, -1, -1
|
| 94 |
+
|
| 95 |
+
def handle_collision(particle_speeds, particle_masses, idx1, idx2, current_step):
|
| 96 |
+
"""Handle a collision between two particles."""
|
| 97 |
+
if particle_masses[idx1] == 0 or particle_masses[idx2] == 0:
|
| 98 |
+
# Skip handling collisions involving massless particles
|
| 99 |
+
return
|
| 100 |
+
|
| 101 |
+
p1 = relativistic_momentum(particle_speeds[idx1, current_step], particle_masses[idx1])
|
| 102 |
+
p2 = relativistic_momentum(particle_speeds[idx2, current_step], particle_masses[idx2])
|
| 103 |
+
|
| 104 |
+
# Calculate velocities after collision using conservation of momentum
|
| 105 |
+
total_momentum = p1 + p2
|
| 106 |
+
total_mass = particle_masses[idx1] + particle_masses[idx2]
|
| 107 |
+
v1_new = (total_momentum / total_mass) * (particle_masses[idx1] / total_mass)
|
| 108 |
+
v2_new = (total_momentum / total_mass) * (particle_masses[idx2] / total_mass)
|
| 109 |
+
|
| 110 |
+
particle_speeds[idx1, current_step], particle_speeds[idx2, current_step] = v1_new, v2_new
|
| 111 |
+
|
| 112 |
+
# Calculate the exact mass of the WIMP
|
| 113 |
+
def calculate_wimp_mass(dark_matter_density, redshift):
|
| 114 |
+
return np.sqrt(2 * dark_matter_density * (1 + redshift)**3)
|
| 115 |
+
|
| 116 |
+
# Calculate the exact mass of the axion
|
| 117 |
+
def calculate_axion_mass(dark_matter_density_GeV):
|
| 118 |
+
return np.sqrt(dark_matter_density_GeV) * 1e-5
|
| 119 |
+
|
| 120 |
+
|
| 121 |
+
# Calculate the redshift
|
| 122 |
+
def calculate_redshift(particle_speed):
|
| 123 |
+
return (1 + particle_speed / c)
|
| 124 |
+
|
| 125 |
+
|
| 126 |
+
|
| 127 |
+
# Simulate the Big Bang with Dark Energy, Dark Matter, Tunneling, Relativistic Effects, Redshift, and Entanglement
|
| 128 |
+
for tunneling_probability in tunneling_probabilities:
|
| 129 |
+
print(f"Simulating for tunneling probability: {tunneling_probability}")
|
| 130 |
+
|
| 131 |
+
# Initialize arrays for simulation
|
| 132 |
+
num_particles = len(particle_masses)
|
| 133 |
+
particle_speeds = np.zeros((num_particles, num_steps)) # 2D array for speeds
|
| 134 |
+
particle_temperatures = np.zeros((num_particles, num_steps)) # 2D array for temperatures
|
| 135 |
+
particle_masses_evolution = np.zeros((num_particles, num_steps)) # 2D array for mass evolution
|
| 136 |
+
tunneling_steps = np.zeros((num_particles, num_steps), dtype=bool) # 2D array for tunneling steps
|
| 137 |
+
particle_momentum = np.zeros((num_particles, num_steps)) # 2D array for momentum
|
| 138 |
+
total_energy = np.zeros(num_steps) # 1D array for total energy of the system
|
| 139 |
+
redshifts = np.zeros((num_particles, num_steps)) # 2D array for redshift
|
| 140 |
+
entanglement_entropies = np.zeros((num_particles, num_steps)) # 2D array for entanglement entropy
|
| 141 |
+
particle_states = np.random.rand(num_particles, num_steps) # Placeholder for particle states
|
| 142 |
+
|
| 143 |
+
# Create an array of masses for each particle
|
| 144 |
+
particle_masses_array = np.array([mass * GeV_to_J for mass in particle_masses.values()])
|
| 145 |
+
|
| 146 |
+
for j, (particle, mass) in enumerate(particle_masses.items()):
|
| 147 |
+
particle_speeds[j, 0] = particle_speed_initial # Initialize speed
|
| 148 |
+
particle_masses_evolution[j, 0] = mass * GeV_to_J # Initialize mass evolution
|
| 149 |
+
|
| 150 |
+
for current_step in range(1, num_steps):
|
| 151 |
+
for j in range(num_particles):
|
| 152 |
+
# Update temperature based on expansion of the universe
|
| 153 |
+
particle_temperatures[j, current_step] = particle_temperatures[j, current_step-1] * (1 - Hubble_constant_SI * t_planck)
|
| 154 |
+
|
| 155 |
+
# Update speed using TSR
|
| 156 |
+
particle_speeds[j, current_step] = update_speed(particle_speeds[j, current_step-1], particle_temperatures[j, current_step], particle_masses_array[j])
|
| 157 |
+
|
| 158 |
+
# Apply tunneling effect
|
| 159 |
+
if np.random.rand() < tunneling_probability:
|
| 160 |
+
particle_speeds[j, current_step] = particle_speeds[j, 0]
|
| 161 |
+
tunneling_steps[j, current_step] = True
|
| 162 |
+
|
| 163 |
+
# Calculate redshift
|
| 164 |
+
redshifts[j, current_step] = (1 + particle_speeds[j, current_step] / c)
|
| 165 |
+
|
| 166 |
+
# Calculate entanglement entropy
|
| 167 |
+
entanglement_entropies[j, current_step] = -np.sum(particle_states[j, current_step] * np.log(particle_states[j, current_step]))
|
| 168 |
+
|
| 169 |
+
# Update mass evolution
|
| 170 |
+
particle_masses_evolution[j, current_step] = particle_masses_evolution[j, current_step-1] * (1 - dark_energy_density * t_planck)
|
| 171 |
+
|
| 172 |
+
# Check for collisions
|
| 173 |
+
collision_detected, idx1, idx2 = check_collision(particle_speeds[:, current_step], collision_distance)
|
| 174 |
+
if collision_detected:
|
| 175 |
+
handle_collision(particle_speeds, particle_masses_array, idx1, idx2, current_step)
|
| 176 |
+
|
| 177 |
+
# Print calculated masses at the end of the simulation
|
| 178 |
+
print(f"Calculated masses at the end of the simulation (Tunneling Probability: {tunneling_probability}):")
|
| 179 |
+
for j, particle in enumerate(particle_masses.keys()):
|
| 180 |
+
print(f"{particle}: {particle_masses_evolution[j, -1] / GeV_to_J:.4e} GeV")
|
| 181 |
+
|
| 182 |
+
# Calculate the exact mass of the WIMP
|
| 183 |
+
wimp_mass = calculate_wimp_mass(dark_matter_density_GeV, calculate_redshift(particle_speeds[-1, -1]))
|
| 184 |
+
|
| 185 |
+
# Calculate the exact mass of the axion
|
| 186 |
+
axion_mass = calculate_axion_mass(dark_matter_density_GeV)
|
| 187 |
+
|
| 188 |
+
# Print the exact masses of the WIMP and axion
|
| 189 |
+
print(f"Exact mass of the WIMP: {wimp_mass / GeV_to_J:.4e} GeV")
|
| 190 |
+
print(f"Exact mass of the axion: {axion_mass / GeV_to_J:.4e} GeV")# Initialize output dictionaries
|
| 191 |
+
outputs = {
|
| 192 |
+
"tunneling_probabilities": tunneling_probabilities.tolist(),
|
| 193 |
+
"speed_ranges": speed_ranges,
|
| 194 |
+
"results": []
|
| 195 |
+
}
|
| 196 |
+
|
| 197 |
+
for speed_range in speed_ranges:
|
| 198 |
+
for tunneling_probability in tunneling_probabilities:
|
| 199 |
+
print(f"Simulating for tunneling probability: {tunneling_probability}, Speed range: {speed_range}")
|
| 200 |
+
|
| 201 |
+
#... (rest of the simulation code remains the same until the WIMP mass calculation)
|
| 202 |
+
|
| 203 |
+
wimp_mass = calculate_wimp_mass(dark_matter_density_GeV, calculate_redshift(particle_speeds[-1, -1]))
|
| 204 |
+
print(f"Exact mass of the WIMP: {wimp_mass / GeV_to_J:.4e} GeV")
|
| 205 |
+
|
| 206 |
+
outputs["results"].append({
|
| 207 |
+
"tunneling_probability": tunneling_probability,
|
| 208 |
+
"speed_range": speed_range,
|
| 209 |
+
"wimp_mass_GeV": wimp_mass / GeV_to_J,
|
| 210 |
+
"wimp_mass_J": wimp_mass,
|
| 211 |
+
"particle_speeds": particle_speeds.tolist()
|
| 212 |
+
})
|
| 213 |
+
|
| 214 |
+
# Save outputs to JSON file
|
| 215 |
+
with open("comprehensive_outputs.json", "w") as f:
|
| 216 |
+
json.dump(outputs, f, indent=4)
|
| 217 |
+
|
| 218 |
+
# Generate correlation plots and statistics
|
| 219 |
+
for speed_range in speed_ranges:
|
| 220 |
+
speed_range_results = [result for result in outputs["results"] if result["speed_range"] == speed_range]
|
| 221 |
+
tunneling_probabilities_speed_range = [result["tunneling_probability"] for result in speed_range_results]
|
| 222 |
+
wimp_masses_speed_range = [result["wimp_mass_GeV"] for result in speed_range_results]
|
| 223 |
+
|
| 224 |
+
plt.figure(figsize=(8, 6))
|
| 225 |
+
plt.scatter(tunneling_probabilities_speed_range, wimp_masses_speed_range)
|
| 226 |
+
plt.xlabel("Tunneling Probability")
|
| 227 |
+
plt.ylabel("Exact Mass of WIMP (GeV)")
|
| 228 |
+
plt.title(f"Correlation between WIMP Mass and Tunneling Probability (Speed range: {speed_range})")
|
| 229 |
+
plt.savefig(f"wimp_mass_correlation_speed_range_{speed_range}.png")
|
| 230 |
+
plt.show()
|
| 231 |
+
|
| 232 |
+
pearson_corr, _ = pearsonr(tunneling_probabilities_speed_range, wimp_masses_speed_range)
|
| 233 |
+
print(f"Pearson correlation coefficient (Speed range: {speed_range}): {pearson_corr:.4f}")
|
| 234 |
+
|
a.py
ADDED
|
@@ -0,0 +1,45 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
# Initialize output dictionaries
|
| 2 |
+
outputs = {
|
| 3 |
+
"tunneling_probabilities": tunneling_probabilities.tolist(),
|
| 4 |
+
"speed_ranges": speed_ranges,
|
| 5 |
+
"results": []
|
| 6 |
+
}
|
| 7 |
+
|
| 8 |
+
for speed_range in speed_ranges:
|
| 9 |
+
for tunneling_probability in tunneling_probabilities:
|
| 10 |
+
print(f"Simulating for tunneling probability: {tunneling_probability}, Speed range: {speed_range}")
|
| 11 |
+
|
| 12 |
+
#... (rest of the simulation code remains the same until the WIMP mass calculation)
|
| 13 |
+
|
| 14 |
+
wimp_mass = calculate_wimp_mass(dark_matter_density_GeV, calculate_redshift(particle_speeds[-1, -1]))
|
| 15 |
+
print(f"Exact mass of the WIMP: {wimp_mass / GeV_to_J:.4e} GeV")
|
| 16 |
+
|
| 17 |
+
outputs["results"].append({
|
| 18 |
+
"tunneling_probability": tunneling_probability,
|
| 19 |
+
"speed_range": speed_range,
|
| 20 |
+
"wimp_mass_GeV": wimp_mass / GeV_to_J,
|
| 21 |
+
"wimp_mass_J": wimp_mass,
|
| 22 |
+
"particle_speeds": particle_speeds.tolist()
|
| 23 |
+
})
|
| 24 |
+
|
| 25 |
+
# Save outputs to JSON file
|
| 26 |
+
with open("comprehensive_outputs.json", "w") as f:
|
| 27 |
+
json.dump(outputs, f, indent=4)
|
| 28 |
+
|
| 29 |
+
# Generate correlation plots and statistics
|
| 30 |
+
for speed_range in speed_ranges:
|
| 31 |
+
speed_range_results = [result for result in outputs["results"] if result["speed_range"] == speed_range]
|
| 32 |
+
tunneling_probabilities_speed_range = [result["tunneling_probability"] for result in speed_range_results]
|
| 33 |
+
wimp_masses_speed_range = [result["wimp_mass_GeV"] for result in speed_range_results]
|
| 34 |
+
|
| 35 |
+
plt.figure(figsize=(8, 6))
|
| 36 |
+
plt.scatter(tunneling_probabilities_speed_range, wimp_masses_speed_range)
|
| 37 |
+
plt.xlabel("Tunneling Probability")
|
| 38 |
+
plt.ylabel("Exact Mass of WIMP (GeV)")
|
| 39 |
+
plt.title(f"Correlation between WIMP Mass and Tunneling Probability (Speed range: {speed_range})")
|
| 40 |
+
plt.savefig(f"wimp_mass_correlation_speed_range_{speed_range}.png")
|
| 41 |
+
plt.show()
|
| 42 |
+
|
| 43 |
+
pearson_corr, _ = pearsonr(tunneling_probabilities_speed_range, wimp_masses_speed_range)
|
| 44 |
+
print(f"Pearson correlation coefficient (Speed range: {speed_range}): {pearson_corr:.4f}")
|
| 45 |
+
|
app.py
CHANGED
|
@@ -1,283 +1,129 @@
|
|
| 1 |
-
import
|
| 2 |
import pandas as pd
|
| 3 |
-
import
|
| 4 |
-
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 5 |
import streamlit as st
|
| 6 |
|
| 7 |
x = st.slider('Select a value')
|
| 8 |
st.write(x, 'squared is', x * x)
|
| 9 |
|
| 10 |
-
#
|
| 11 |
-
|
| 12 |
-
E_mc2 = c**2 # Mass-energy equivalence in J/kg
|
| 13 |
-
TSR = E_mc2 / (1.38e-23) # Temperature to Speed Ratio in K/m/s
|
| 14 |
-
alpha = 1.0 # Proportional constant for TSR
|
| 15 |
-
Q = 2 ** (1 / 12) # Fractal structure parameter
|
| 16 |
-
dark_energy_density = 5.96e-27 # Density of dark energy in kg/m^3
|
| 17 |
-
dark_matter_density = 2.25e-27 # Density of dark matter in kg/m^3
|
| 18 |
-
collision_distance = 1e-10 # Distance for collision detection
|
| 19 |
-
Hubble_constant = 70.0 # km/s/Mpc (approximation)
|
| 20 |
-
Hubble_constant_SI = Hubble_constant * 1000 / 3.086e22 # Convert to SI units (s^-1)
|
| 21 |
-
|
| 22 |
-
# Convert dark matter density to GeV/m³
|
| 23 |
-
dark_matter_density_GeV = dark_matter_density / 1.60217662e-10
|
| 24 |
-
|
| 25 |
-
# Initial conditions
|
| 26 |
-
temperature_initial = 1.0 # Planck temperature in K
|
| 27 |
-
particle_density_initial = 5.16e96 # Planck density in kg/m^3
|
| 28 |
-
particle_speed_initial = TSR * temperature_initial # Initial speed based on TSR
|
| 29 |
-
|
| 30 |
-
# Simulation time
|
| 31 |
-
t_planck = 5.39e-44 # Planck time in s
|
| 32 |
-
t_simulation = t_planck * 1e5 # Shorter timescale for simulation
|
| 33 |
-
|
| 34 |
-
# Updated particle masses (in GeV)
|
| 35 |
-
particle_masses = {
|
| 36 |
-
"up": 2.3e-3,
|
| 37 |
-
"down": 4.8e-3,
|
| 38 |
-
"charm": 1.28,
|
| 39 |
-
"strange": 0.095,
|
| 40 |
-
"top": 173.0,
|
| 41 |
-
"bottom": 4.18,
|
| 42 |
-
"electron": 5.11e-4,
|
| 43 |
-
"muon": 1.05e-1,
|
| 44 |
-
"tau": 1.78,
|
| 45 |
-
"photon": 0,
|
| 46 |
-
"electron_neutrino": 0, # Neutrinos have very small masses
|
| 47 |
-
"muon_neutrino": 0,
|
| 48 |
-
"tau_neutrino": 0,
|
| 49 |
-
"W_boson": 80.379,
|
| 50 |
-
"Z_boson": 91.1876,
|
| 51 |
-
"Higgs_boson": 125.1,
|
| 52 |
-
"gluon": 0, # Massless
|
| 53 |
-
"proton": 0.938,
|
| 54 |
-
"neutron": 0.939,
|
| 55 |
-
"pion_plus": 0.140,
|
| 56 |
-
"pion_zero": 0.135,
|
| 57 |
-
"kaon_plus": 0.494,
|
| 58 |
-
"kaon_zero": 0.498
|
| 59 |
-
}
|
| 60 |
-
|
| 61 |
-
# Conversion factor from GeV to J
|
| 62 |
-
GeV_to_J = 1.60217662e-10
|
| 63 |
-
|
| 64 |
-
# Simulation setup
|
| 65 |
-
num_steps = int(t_simulation / t_planck)
|
| 66 |
-
|
| 67 |
-
import numpy as np
|
| 68 |
-
def generate_combined_tunneling_probabilities(start, stop, step_odd, step_even):
|
| 69 |
-
"""Generates a combined sequence of tunneling probabilities with alternating odd and even decimal places."""
|
| 70 |
-
odd_tp = np.arange(start, stop, step_odd)
|
| 71 |
-
even_tp = np.arange(start, stop, step_even)
|
| 72 |
-
combined_tp = np.concatenate((odd_tp, even_tp))
|
| 73 |
-
return combined_tp
|
| 74 |
-
# Example usage:
|
| 75 |
-
tunneling_probabilities = generate_combined_tunneling_probabilities(0.1, 1.5, 0.02, 0.01)
|
| 76 |
-
print(tunneling_probabilities)
|
| 77 |
-
# Create a directory to store the data
|
| 78 |
-
data_dir = "big_bang_simulation_data"
|
| 79 |
-
os.makedirs(data_dir, exist_ok=True)
|
| 80 |
-
|
| 81 |
-
# Functions to incorporate relativistic effects and collisions
|
| 82 |
-
def relativistic_energy(particle_speed, particle_mass):
|
| 83 |
-
epsilon = 1e-15 # A small value to avoid division by zero
|
| 84 |
-
return particle_mass * c**2 / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 85 |
-
|
| 86 |
-
def relativistic_momentum(particle_speed, particle_mass):
|
| 87 |
-
epsilon = 1e-15 # A small value to avoid division by zero
|
| 88 |
-
return particle_mass * particle_speed / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 89 |
-
|
| 90 |
-
def update_speed(current_speed, current_temperature, particle_mass):
|
| 91 |
-
"""Update the speed of a particle based on temperature and mass."""
|
| 92 |
-
return TSR * current_temperature # Update speed using TSR
|
| 93 |
-
|
| 94 |
-
def check_collision(particle_speeds, collision_distance):
|
| 95 |
-
epsilon = 1e-15 # A small value to avoid invalid subtraction
|
| 96 |
-
for j in range(len(particle_speeds)):
|
| 97 |
-
for k in range(j+1, len(particle_speeds)):
|
| 98 |
-
if np.abs(particle_speeds[j] - particle_speeds[k]) < collision_distance + epsilon:
|
| 99 |
-
return True, j, k
|
| 100 |
-
return False, -1, -1
|
| 101 |
-
|
| 102 |
-
def handle_collision(particle_speeds, particle_masses, idx1, idx2, current_step):
|
| 103 |
-
"""Handle a collision between two particles."""
|
| 104 |
-
if particle_masses[idx1] == 0 or particle_masses[idx2] == 0:
|
| 105 |
-
# Skip handling collisions involving massless particles
|
| 106 |
-
return
|
| 107 |
-
|
| 108 |
-
p1 = relativistic_momentum(particle_speeds[idx1, current_step], particle_masses[idx1])
|
| 109 |
-
p2 = relativistic_momentum(particle_speeds[idx2, current_step], particle_masses[idx2])
|
| 110 |
-
|
| 111 |
-
# Calculate velocities after collision using conservation of momentum
|
| 112 |
-
total_momentum = p1 + p2
|
| 113 |
-
total_mass = particle_masses[idx1] + particle_masses[idx2]
|
| 114 |
-
v1_new = (total_momentum / total_mass) * (particle_masses[idx1] / total_mass)
|
| 115 |
-
v2_new = (total_momentum / total_mass) * (particle_masses[idx2] / total_mass)
|
| 116 |
-
|
| 117 |
-
particle_speeds[idx1, current_step], particle_speeds[idx2, current_step] = v1_new, v2_new
|
| 118 |
-
|
| 119 |
-
|
| 120 |
-
def calculate_redshift(particle_speed):
|
| 121 |
-
return (1 + particle_speed / c)
|
| 122 |
-
# Calculate the exact mass of the WIMP
|
| 123 |
-
def calculate_wimp_mass(dark_matter_density_GeV, redshift):
|
| 124 |
-
return np.sqrt(2 * dark_matter_density_GeV * (1 + redshift)**3)
|
| 125 |
-
|
| 126 |
-
# Calculate the exact mass of the axion
|
| 127 |
-
def calculate_axion_mass(dark_matter_density_GeV):
|
| 128 |
-
return np.sqrt(dark_matter_density_GeV) * 1e-5
|
| 129 |
-
|
| 130 |
-
# Calculate the exact mass of the graviton
|
| 131 |
-
def calculate_graviton_mass(dark_matter_density_GeV):
|
| 132 |
-
return 0 # Graviton is massless
|
| 133 |
-
|
| 134 |
-
# Calculate the exact mass of the muon g-2
|
| 135 |
-
def calculate_muon_g2_mass(dark_matter_density_GeV):
|
| 136 |
-
return 1.05e-1 # Muon mass
|
| 137 |
|
| 138 |
-
#
|
| 139 |
-
def
|
| 140 |
-
|
|
|
|
| 141 |
|
| 142 |
-
#
|
| 143 |
-
|
| 144 |
-
|
|
|
|
| 145 |
|
| 146 |
-
|
| 147 |
-
|
| 148 |
-
|
| 149 |
-
particle_temperatures = np.zeros((num_particles, num_steps)) # 2D array for temperatures
|
| 150 |
-
particle_masses_evolution = np.zeros((num_particles, num_steps)) # 2D array for mass evolution
|
| 151 |
-
tunneling_steps = np.zeros((num_particles, num_steps), dtype=bool) # 2D array for tunneling steps
|
| 152 |
-
particle_momentum = np.zeros((num_particles, num_steps)) # 2D array for momentum
|
| 153 |
-
total_energy = np.zeros(num_steps) # 1D array for total energy of the system
|
| 154 |
-
redshifts = np.zeros((num_particles, num_steps)) # 2D array for redshift
|
| 155 |
-
entanglement_entropies = np.zeros((num_particles, num_steps)) # 2D array for entanglement entropy
|
| 156 |
-
particle_states = np.random.rand(num_particles, num_steps) # Placeholder for particle states
|
| 157 |
|
| 158 |
-
|
| 159 |
-
|
|
|
|
| 160 |
|
| 161 |
-
|
| 162 |
-
|
| 163 |
-
particle_masses_evolution[j, 0] = mass * GeV_to_J # Initialize mass evolution
|
| 164 |
|
| 165 |
-
|
| 166 |
-
|
| 167 |
-
|
| 168 |
-
|
| 169 |
|
| 170 |
-
|
| 171 |
-
particle_speeds[j, current_step] = update_speed(particle_speeds[j, current_step-1], particle_temperatures[j, current_step], particle_masses_array[j])
|
| 172 |
|
| 173 |
-
|
| 174 |
-
|
| 175 |
-
|
| 176 |
-
tunneling_steps[j, current_step] = True
|
| 177 |
-
|
| 178 |
-
# Calculate redshift
|
| 179 |
-
redshifts[j, current_step] = (1 + particle_speeds[j, current_step] / c)
|
| 180 |
-
|
| 181 |
-
# Calculate entanglement entropy
|
| 182 |
-
entanglement_entropies[j, current_step] = -np.sum(particle_states[j, current_step] * np.log(particle_states[j, current_step]))
|
| 183 |
-
|
| 184 |
-
# Update mass evolution
|
| 185 |
-
particle_masses_evolution[j, current_step] = particle_masses_evolution[j, current_step-1] * (1 - dark_energy_density * t_planck)
|
| 186 |
-
|
| 187 |
-
# Check for collisions
|
| 188 |
-
collision_detected, idx1, idx2 = check_collision(particle_speeds[:, current_step], collision_distance)
|
| 189 |
-
if collision_detected:
|
| 190 |
-
handle_collision(particle_speeds, particle_masses_array, idx1, idx2, current_step)
|
| 191 |
-
|
| 192 |
-
# Print calculated masses at the end of the simulation
|
| 193 |
-
print(f"Calculated masses at the end of the simulation (Tunneling Probability: {tunneling_probability}):")
|
| 194 |
-
for j, particle in enumerate(particle_masses.keys()):
|
| 195 |
-
print(f"{particle}: {particle_masses_evolution[j, -1] / GeV_to_J:.4e} GeV")
|
| 196 |
-
|
| 197 |
-
# Calculate the exact masses of the WIMP, axion, graviton, muon g-2, and preon
|
| 198 |
-
wimp_mass = calculate_wimp_mass(dark_matter_density_GeV, calculate_redshift(particle_speeds[-1, -1]))
|
| 199 |
-
axion_mass = calculate_axion_mass(dark_matter_density_GeV)
|
| 200 |
-
graviton_mass = calculate_graviton_mass(dark_matter_density_GeV)
|
| 201 |
-
muon_g2_mass = calculate_muon_g2_mass(dark_matter_density_GeV)
|
| 202 |
-
preon_mass = calculate_preon_mass(dark_matter_density_GeV)
|
| 203 |
-
|
| 204 |
-
# Print the exact masses of the WIMP and axion
|
| 205 |
-
print(f"Exact mass of the WIMP: {wimp_mass / GeV_to_J:.4e} GeV")
|
| 206 |
-
print(f"Exact mass of the axion: {axion_mass / GeV_to_J:.4e} GeV")
|
| 207 |
-
print(f"Exact mass of the graviton_mass: {graviton_mass/ GeV_to_J:.4e} GeV")
|
| 208 |
-
import numpy as np
|
| 209 |
-
import matplotlib.pyplot as plt
|
| 210 |
-
|
| 211 |
-
# Define the correlation matrix
|
| 212 |
-
correlation_matrix = np.array([
|
| 213 |
-
[1]
|
| 214 |
])
|
| 215 |
|
| 216 |
-
|
| 217 |
-
|
| 218 |
-
|
| 219 |
-
|
| 220 |
-
|
| 221 |
-
|
| 222 |
-
|
| 223 |
-
|
| 224 |
-
|
| 225 |
-
|
| 226 |
-
|
| 227 |
-
|
| 228 |
-
|
| 229 |
-
|
| 230 |
-
|
| 231 |
-
|
| 232 |
-
|
| 233 |
-
|
| 234 |
-
|
| 235 |
-
|
| 236 |
-
|
| 237 |
-
|
| 238 |
-
|
| 239 |
-
|
| 240 |
-
|
| 241 |
-
|
| 242 |
-
|
| 243 |
-
|
| 244 |
-
|
| 245 |
-
|
| 246 |
-
|
| 247 |
-
|
| 248 |
-
|
| 249 |
-
|
| 250 |
-
|
| 251 |
-
|
| 252 |
-
|
| 253 |
-
|
| 254 |
-
|
| 255 |
-
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 256 |
fig, ax = plt.subplots()
|
| 257 |
-
|
| 258 |
-
|
| 259 |
-
ax.
|
| 260 |
-
ax.
|
| 261 |
-
|
| 262 |
-
|
| 263 |
-
|
| 264 |
-
|
| 265 |
-
|
| 266 |
-
|
| 267 |
-
|
| 268 |
-
|
| 269 |
-
|
| 270 |
-
|
| 271 |
plt.show()
|
| 272 |
-
|
| 273 |
-
# Create a dictionary to store the trends
|
| 274 |
-
trends = {
|
| 275 |
-
'Correlation Matrix': correlation_matrix,
|
| 276 |
-
'WIMP Mass Values': [wimp_mass_odd, wimp_mass_even],
|
| 277 |
-
'Correlation between WIMP Mass and itself': corr_mass_mass
|
| 278 |
-
}
|
| 279 |
-
|
| 280 |
-
# Print the trends
|
| 281 |
-
print("\nTrends:")
|
| 282 |
-
for key, value in trends.items():
|
| 283 |
-
print(key, ":", value)
|
|
|
|
| 1 |
+
import streamlit as st
|
| 2 |
import pandas as pd
|
| 3 |
+
import numpy as np
|
| 4 |
+
st.title('Quantum Convergence Theory - ToE')
|
| 5 |
+
|
| 6 |
+
import matplotlib.pyplot as plt
|
| 7 |
+
from matplotlib.animation import FuncAnimation
|
| 8 |
+
import cupy as cp
|
| 9 |
+
from tqdm import tqdm
|
| 10 |
+
import plotly.graph_objects as go
|
| 11 |
import streamlit as st
|
| 12 |
|
| 13 |
x = st.slider('Select a value')
|
| 14 |
st.write(x, 'squared is', x * x)
|
| 15 |
|
| 16 |
+
# Define the twelfth root of two
|
| 17 |
+
Q = 2 ** (1/12)
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
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|
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|
|
| 18 |
|
| 19 |
+
# Define the wave function of the universe with variants (using CuPy)
|
| 20 |
+
def wave_function_cupy(x, t, scale=1.0, phase_shift=0.0):
|
| 21 |
+
denominator = 2 * (t**2 + 1e-10) # Add a small value to avoid division by zero
|
| 22 |
+
return scale * Q * cp.exp(-x**2 / denominator) * cp.exp(-1j * (t + phase_shift))
|
| 23 |
|
| 24 |
+
# Simulation parameters
|
| 25 |
+
x = np.linspace(-10, 10, 100)
|
| 26 |
+
t = np.linspace(0, 10, 100)
|
| 27 |
+
X, T = np.meshgrid(x, t)
|
| 28 |
|
| 29 |
+
# Convert numpy arrays to CuPy arrays
|
| 30 |
+
X_cupy = cp.asarray(X)
|
| 31 |
+
T_cupy = cp.asarray(T)
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 32 |
|
| 33 |
+
# Variants parameters
|
| 34 |
+
scales = [0.5, 1.0, 1.5] # Different scaling factors
|
| 35 |
+
phase_shifts = [0, np.pi/4, np.pi/2] # Different phase shifts
|
| 36 |
|
| 37 |
+
# Initialize a 3D array to store results
|
| 38 |
+
wave_functions_3d = np.zeros((len(scales), len(phase_shifts), len(x), len(t)), dtype=complex)
|
|
|
|
| 39 |
|
| 40 |
+
# Simulate with variants and store results in the 3D array
|
| 41 |
+
for i, scale in enumerate(scales):
|
| 42 |
+
for j, phase_shift in enumerate(phase_shifts):
|
| 43 |
+
wave_functions_3d[i, j, :, :] = cp.asnumpy(wave_function_cupy(X_cupy, T_cupy, scale, phase_shift))
|
| 44 |
|
| 45 |
+
# --- Plotly Interactive Visualization ---
|
|
|
|
| 46 |
|
| 47 |
+
# Create the figure
|
| 48 |
+
fig = go.Figure(data=[
|
| 49 |
+
go.Surface(x=x, y=t, z=np.abs(wave_functions_3d[0, 0, :, :])**2)
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 50 |
])
|
| 51 |
|
| 52 |
+
fig.update_layout(
|
| 53 |
+
title="Wave Function of the Universe",
|
| 54 |
+
scene=dict(
|
| 55 |
+
xaxis_title="x",
|
| 56 |
+
yaxis_title="t",
|
| 57 |
+
zaxis_title="|ψ(x,t)|^2"
|
| 58 |
+
),
|
| 59 |
+
)
|
| 60 |
+
|
| 61 |
+
# Add Scale Slider
|
| 62 |
+
fig.update_layout(
|
| 63 |
+
sliders=[
|
| 64 |
+
dict(
|
| 65 |
+
active=True,
|
| 66 |
+
currentvalue=dict(
|
| 67 |
+
prefix="Scale: ",
|
| 68 |
+
font=dict(size=12)
|
| 69 |
+
),
|
| 70 |
+
steps=[
|
| 71 |
+
dict(
|
| 72 |
+
method="update",
|
| 73 |
+
args=[
|
| 74 |
+
{"z": [np.abs(wave_functions_3d[i, 0, :, :])**2]} # Update z data
|
| 75 |
+
],
|
| 76 |
+
label=f"Scale: {scales[i]:.2f}" # Label for step values
|
| 77 |
+
) for i in range(len(scales))
|
| 78 |
+
],
|
| 79 |
+
pad=dict(t=50),
|
| 80 |
+
len=0.9, # Length of the slider
|
| 81 |
+
x=0.1, # X position of the slider
|
| 82 |
+
y=0.1, # Y position of the slider
|
| 83 |
+
),
|
| 84 |
+
dict(
|
| 85 |
+
active=True,
|
| 86 |
+
currentvalue=dict(
|
| 87 |
+
prefix="Phase Shift: ",
|
| 88 |
+
font=dict(size=12)
|
| 89 |
+
),
|
| 90 |
+
steps=[
|
| 91 |
+
dict(
|
| 92 |
+
method="update",
|
| 93 |
+
args=[
|
| 94 |
+
{"z": [np.abs(wave_functions_3d[0, j, :, :])**2]} # Update z data
|
| 95 |
+
],
|
| 96 |
+
label=f"Phase Shift: {phase_shifts[j]:.2f}" # Label for step values
|
| 97 |
+
) for j in range(len(phase_shifts))
|
| 98 |
+
],
|
| 99 |
+
pad=dict(t=50),
|
| 100 |
+
len=0.9, # Length of the slider
|
| 101 |
+
x=0.1, # X position of the slider
|
| 102 |
+
y=0.3, # Y position of the slider
|
| 103 |
+
)
|
| 104 |
+
]
|
| 105 |
+
)
|
| 106 |
+
|
| 107 |
+
fig.show()
|
| 108 |
+
|
| 109 |
+
# --- End of Plotly ---
|
| 110 |
+
|
| 111 |
+
# --- Matplotlib Animation ---
|
| 112 |
+
|
| 113 |
+
# Animation
|
| 114 |
fig, ax = plt.subplots()
|
| 115 |
+
im = ax.imshow(np.abs(wave_functions_3d[0, 0, :, :]) ** 2, extent=[-10, 10, 0, 10], aspect='auto', cmap='viridis')
|
| 116 |
+
ax.set_xlabel('x')
|
| 117 |
+
ax.set_ylabel('t')
|
| 118 |
+
ax.set_title('Wave Function of the Universe')
|
| 119 |
+
cbar = fig.colorbar(im, ax=ax, label='|ψ(x,t)|^2')
|
| 120 |
+
|
| 121 |
+
def update(frame):
|
| 122 |
+
i, j = divmod(frame, len(phase_shifts)) # Get the index for the 3D array
|
| 123 |
+
im.set_array(np.abs(wave_functions_3d[i, j, :, :]) ** 2) # Update with the correct frame
|
| 124 |
+
ax.set_title(f'Wave Function at Scale: {scales[i]}, Phase Shift: {phase_shifts[j]:.2f}')
|
| 125 |
+
return im,
|
| 126 |
+
|
| 127 |
+
ani = FuncAnimation(fig, update, frames=len(scales) * len(phase_shifts), blit=True)
|
| 128 |
+
ani.save('wave_function_animation.gif', writer='pillow')
|
| 129 |
plt.show()
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
js.py
ADDED
|
@@ -0,0 +1,40 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import json
|
| 2 |
+
import pandas as pd
|
| 3 |
+
import matplotlib.pyplot as plt
|
| 4 |
+
import seaborn as sns
|
| 5 |
+
|
| 6 |
+
# Function to load JSON data
|
| 7 |
+
def load_json_data(json_file):
|
| 8 |
+
with open(json_file, 'r') as file:
|
| 9 |
+
return json.load(file)
|
| 10 |
+
|
| 11 |
+
# Load multiple JSON files into a DataFrame
|
| 12 |
+
data_files = [
|
| 13 |
+
'.\\Downloads\\big_bang_simulation_data\\big_bang_simulation_data_0.01.json',
|
| 14 |
+
'.\\Downloads\\big_bang_simulation_data\\big_bang_simulation_data_0.02.json',
|
| 15 |
+
'.\\Downloads\\big_bang_simulation_data\\big_bang_simulation_data_0.03.json',
|
| 16 |
+
# Add more files as needed
|
| 17 |
+
]
|
| 18 |
+
|
| 19 |
+
data_list = [load_json_data(f) for f in data_files]
|
| 20 |
+
|
| 21 |
+
# Extract relevant data into a DataFrame
|
| 22 |
+
df = pd.DataFrame([
|
| 23 |
+
{
|
| 24 |
+
'tunneling_probability': data['tunneling_probability'],
|
| 25 |
+
'particle_mass_up': data['particle_masses_evolution'][0][-1],
|
| 26 |
+
'particle_mass_down': data['particle_masses_evolution'][1][-1],
|
| 27 |
+
# Add more particles as needed
|
| 28 |
+
'particle_speed': data['particle_speeds'][0][-1], # Example particle speed
|
| 29 |
+
'particle_temperature': data['particle_temperatures'][0][-1], # Example particle temperature
|
| 30 |
+
}
|
| 31 |
+
for data in data_list
|
| 32 |
+
])
|
| 33 |
+
|
| 34 |
+
# Assume df is your DataFrame with simulation results
|
| 35 |
+
correlation_matrix = df.corr()
|
| 36 |
+
|
| 37 |
+
plt.figure(figsize=(10, 8))
|
| 38 |
+
sns.heatmap(correlation_matrix, annot=True, cmap='coolwarm')
|
| 39 |
+
plt.title('Correlation Matrix')
|
| 40 |
+
plt.show()
|
js1.py
ADDED
|
@@ -0,0 +1,49 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import json
|
| 2 |
+
import os
|
| 3 |
+
import pandas as pd
|
| 4 |
+
import matplotlib.pyplot as plt
|
| 5 |
+
import seaborn as sns
|
| 6 |
+
|
| 7 |
+
# Function to load JSON data
|
| 8 |
+
def load_json_data(json_file):
|
| 9 |
+
with open(json_file, 'r') as file:
|
| 10 |
+
return json.load(file)
|
| 11 |
+
|
| 12 |
+
# Directory containing the JSON files
|
| 13 |
+
data_dir = '.\\Documents\\big_bang_simulation_data\\'
|
| 14 |
+
|
| 15 |
+
# List all JSON files in the directory
|
| 16 |
+
data_files = [os.path.join(data_dir, f) for f in os.listdir(data_dir) if f.endswith('.json')]
|
| 17 |
+
|
| 18 |
+
# Load multiple JSON files into a DataFrame
|
| 19 |
+
data_list = [load_json_data(f) for f in data_files]
|
| 20 |
+
|
| 21 |
+
# Extract relevant data into a DataFrame
|
| 22 |
+
df = pd.DataFrame([
|
| 23 |
+
{
|
| 24 |
+
'tunneling_probability': data['tunneling_probability'],
|
| 25 |
+
'particle_mass_up': data['particle_masses_evolution'][0][-1],
|
| 26 |
+
'particle_mass_down': data['particle_masses_evolution'][1][-1],
|
| 27 |
+
'particle_mass_charm': data['particle_masses_evolution'][2][-1],
|
| 28 |
+
'particle_mass_strange': data['particle_masses_evolution'][3][-1],
|
| 29 |
+
'particle_mass_top': data['particle_masses_evolution'][4][-1],
|
| 30 |
+
'particle_mass_bottom': data['particle_masses_evolution'][5][-1],
|
| 31 |
+
'particle_mass_electron': data['particle_masses_evolution'][6][-1],
|
| 32 |
+
'particle_mass_muon': data['particle_masses_evolution'][7][-1],
|
| 33 |
+
'particle_mass_tau': data['particle_masses_evolution'][8][-1],
|
| 34 |
+
'particle_mass_photon': data['particle_masses_evolution'][9][-1],
|
| 35 |
+
'particle_speed': data['particle_speeds'][0][-1],
|
| 36 |
+
'particle_temperature': data['particle_temperatures'][0][-1],
|
| 37 |
+
}
|
| 38 |
+
for data in data_list
|
| 39 |
+
])
|
| 40 |
+
|
| 41 |
+
# Compute correlations
|
| 42 |
+
correlation_matrix = df.corr()
|
| 43 |
+
|
| 44 |
+
# Adjust figure size for better visibility
|
| 45 |
+
plt.figure(figsize=(12, 10))
|
| 46 |
+
sns.heatmap(correlation_matrix, annot=True, cmap='coolwarm')
|
| 47 |
+
plt.title('Correlation Matrix')
|
| 48 |
+
plt.show()
|
| 49 |
+
|
js2.py
ADDED
|
@@ -0,0 +1,117 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import json
|
| 2 |
+
import os
|
| 3 |
+
import pandas as pd
|
| 4 |
+
import matplotlib.pyplot as plt
|
| 5 |
+
import seaborn as sns
|
| 6 |
+
from sklearn.decomposition import PCA
|
| 7 |
+
|
| 8 |
+
# Function to load JSON data
|
| 9 |
+
def load_json_data(json_file):
|
| 10 |
+
with open(json_file, 'r') as file:
|
| 11 |
+
return json.load(file)
|
| 12 |
+
|
| 13 |
+
# Directory containing the JSON files
|
| 14 |
+
data_dir = '.\\Documents\\big_bang_simulation_data\\'
|
| 15 |
+
|
| 16 |
+
# List all JSON files in the directory
|
| 17 |
+
data_files = [os.path.join(data_dir, f) for f in os.listdir(data_dir) if f.endswith('.json')]
|
| 18 |
+
|
| 19 |
+
# Load multiple JSON files into a DataFrame
|
| 20 |
+
data_list = [load_json_data(f) for f in data_files]
|
| 21 |
+
|
| 22 |
+
# Extract relevant data into a DataFrame
|
| 23 |
+
df = pd.DataFrame([
|
| 24 |
+
{
|
| 25 |
+
'tunneling_probability': data['tunneling_probability'],
|
| 26 |
+
'particle_mass_up': data['particle_masses_evolution'][0][-1],
|
| 27 |
+
'particle_mass_down': data['particle_masses_evolution'][1][-1],
|
| 28 |
+
'particle_mass_charm': data['particle_masses_evolution'][2][-1],
|
| 29 |
+
'particle_mass_strange': data['particle_masses_evolution'][3][-1],
|
| 30 |
+
'particle_mass_top': data['particle_masses_evolution'][4][-1],
|
| 31 |
+
'particle_mass_bottom': data['particle_masses_evolution'][5][-1],
|
| 32 |
+
'particle_mass_electron': data['particle_masses_evolution'][6][-1],
|
| 33 |
+
'particle_mass_muon': data['particle_masses_evolution'][7][-1],
|
| 34 |
+
'particle_mass_tau': data['particle_masses_evolution'][8][-1],
|
| 35 |
+
'particle_mass_photon': data['particle_masses_evolution'][9][-1],
|
| 36 |
+
'particle_speed': data['particle_speeds'][0][-1],
|
| 37 |
+
'particle_temperature': data['particle_temperatures'][0][-1],
|
| 38 |
+
}
|
| 39 |
+
for data in data_list
|
| 40 |
+
])
|
| 41 |
+
|
| 42 |
+
# Scatter Plot: Tunneling Probability vs Up Quark Mass
|
| 43 |
+
plt.figure(figsize=(8, 6))
|
| 44 |
+
sns.scatterplot(x='tunneling_probability', y='particle_mass_up', data=df)
|
| 45 |
+
plt.title('Tunneling Probability vs Up Quark Mass')
|
| 46 |
+
plt.xlabel('Tunneling Probability')
|
| 47 |
+
plt.ylabel('Up Quark Mass (GeV)')
|
| 48 |
+
plt.show()
|
| 49 |
+
|
| 50 |
+
# Scatter Plot: Particle Temperature vs Speed
|
| 51 |
+
plt.figure(figsize=(8, 6))
|
| 52 |
+
sns.scatterplot(x='particle_temperature', y='particle_speed', data=df)
|
| 53 |
+
plt.title('Particle Temperature vs Speed')
|
| 54 |
+
plt.xlabel('Temperature (K)')
|
| 55 |
+
plt.ylabel('Speed (m/s)')
|
| 56 |
+
plt.show()
|
| 57 |
+
|
| 58 |
+
# Line Graph: Evolution of Up Quark Mass Over Time
|
| 59 |
+
time_steps = range(len(data_list[0]['particle_masses_evolution'][0]))
|
| 60 |
+
plt.figure(figsize=(10, 6))
|
| 61 |
+
for data in data_list:
|
| 62 |
+
plt.plot(time_steps, data['particle_masses_evolution'][0], label=f"Tunneling Probability: {data['tunneling_probability']:.2f}")
|
| 63 |
+
plt.title('Evolution of Up Quark Mass Over Time')
|
| 64 |
+
plt.xlabel('Time Steps')
|
| 65 |
+
plt.ylabel('Up Quark Mass (GeV)')
|
| 66 |
+
plt.legend()
|
| 67 |
+
plt.show()
|
| 68 |
+
|
| 69 |
+
# Dimensionality Reduction: PCA
|
| 70 |
+
features = ['particle_mass_up', 'particle_mass_down', 'particle_mass_charm', 'particle_mass_strange', 'particle_mass_top', 'particle_mass_bottom', 'particle_mass_electron', 'particle_mass_muon', 'particle_mass_tau', 'particle_mass_photon', 'particle_speed', 'particle_temperature']
|
| 71 |
+
X = df[features]
|
| 72 |
+
pca = PCA(n_components=2)
|
| 73 |
+
principal_components = pca.fit_transform(X)
|
| 74 |
+
pca_df = pd.DataFrame(data=principal_components, columns=['PC1', 'PC2'])
|
| 75 |
+
|
| 76 |
+
# PCA Plot
|
| 77 |
+
plt.figure(figsize=(8, 6))
|
| 78 |
+
sns.scatterplot(x='PC1', y='PC2', data=pca_df, hue=df['tunneling_probability'], palette='viridis')
|
| 79 |
+
plt.title('PCA of Particle Properties')
|
| 80 |
+
plt.xlabel('Principal Component 1')
|
| 81 |
+
plt.ylabel('Principal Component 2')
|
| 82 |
+
plt.show()
|
| 83 |
+
|
| 84 |
+
# Investigate correlations in detail
|
| 85 |
+
correlation_matrix = df.corr()
|
| 86 |
+
plt.figure(figsize=(12, 10))
|
| 87 |
+
sns.heatmap(correlation_matrix, annot=True, cmap='coolwarm')
|
| 88 |
+
plt.title('Detailed Correlation Matrix')
|
| 89 |
+
plt.show()
|
| 90 |
+
|
| 91 |
+
# Identify highly correlated pairs
|
| 92 |
+
correlated_pairs = correlation_matrix.unstack().sort_values(kind="quicksort")
|
| 93 |
+
highly_correlated_pairs = correlated_pairs[(abs(correlated_pairs) > 0.8) & (abs(correlated_pairs) < 1)]
|
| 94 |
+
|
| 95 |
+
# Print highly correlated pairs
|
| 96 |
+
print("Highly Correlated Pairs:")
|
| 97 |
+
print(highly_correlated_pairs)
|
| 98 |
+
|
| 99 |
+
# Considering additional variables if available
|
| 100 |
+
df['particle_momentum'] = [...] # Add momentum data if available
|
| 101 |
+
df['particle_energy'] = [...] # Add energy data if available
|
| 102 |
+
|
| 103 |
+
# Re-run PCA with additional variables
|
| 104 |
+
features = ['particle_mass_up', 'particle_mass_down', 'particle_mass_charm', 'particle_mass_strange', 'particle_mass_top', 'particle_mass_bottom', 'particle_mass_electron', 'particle_mass_muon', 'particle_mass_tau', 'particle_mass_photon', 'particle_speed', 'particle_temperature', 'particle_momentum', 'particle_energy']
|
| 105 |
+
X = df[features]
|
| 106 |
+
pca = PCA(n_components=2)
|
| 107 |
+
principal_components = pca.fit_transform(X)
|
| 108 |
+
pca_df = pd.DataFrame(data=principal_components, columns=['PC1', 'PC2'])
|
| 109 |
+
|
| 110 |
+
# Plot updated PCA results
|
| 111 |
+
plt.figure(figsize=(8, 6))
|
| 112 |
+
sns.scatterplot(x='PC1', y='PC2', data=pca_df, hue=df['tunneling_probability'], palette='viridis')
|
| 113 |
+
plt.title('PCA of Particle Properties with Additional Variables')
|
| 114 |
+
plt.xlabel('Principal Component 1')
|
| 115 |
+
plt.ylabel('Principal Component 2')
|
| 116 |
+
plt.show()
|
| 117 |
+
|
js3.py
ADDED
|
@@ -0,0 +1,79 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import json
|
| 2 |
+
import os
|
| 3 |
+
import pandas as pd
|
| 4 |
+
import matplotlib.pyplot as plt
|
| 5 |
+
import seaborn as sns
|
| 6 |
+
from sklearn.decomposition import PCA
|
| 7 |
+
|
| 8 |
+
# Function to load JSON data
|
| 9 |
+
def load_json_data(json_file):
|
| 10 |
+
with open(json_file, 'r') as file:
|
| 11 |
+
return json.load(file)
|
| 12 |
+
|
| 13 |
+
# Directory containing the JSON files
|
| 14 |
+
data_dir = '.\\Documents\\big_bang_simulation_data\\'
|
| 15 |
+
|
| 16 |
+
# List all JSON files in the directory
|
| 17 |
+
data_files = [os.path.join(data_dir, f) for f in os.listdir(data_dir) if f.endswith('.json')]
|
| 18 |
+
|
| 19 |
+
# Load multiple JSON files into a DataFrame
|
| 20 |
+
data_list = []
|
| 21 |
+
for f in data_files:
|
| 22 |
+
data = load_json_data(f)
|
| 23 |
+
data_list.append({
|
| 24 |
+
'tunneling_probability': data['tunneling_probability'],
|
| 25 |
+
'particle_mass_up': data['particle_masses_evolution'][0][-1],
|
| 26 |
+
'particle_mass_down': data['particle_masses_evolution'][1][-1],
|
| 27 |
+
'particle_mass_charm': data['particle_masses_evolution'][2][-1],
|
| 28 |
+
'particle_mass_strange': data['particle_masses_evolution'][3][-1],
|
| 29 |
+
'particle_mass_top': data['particle_masses_evolution'][4][-1],
|
| 30 |
+
'particle_mass_bottom': data['particle_masses_evolution'][5][-1],
|
| 31 |
+
'particle_mass_electron': data['particle_masses_evolution'][6][-1],
|
| 32 |
+
'particle_mass_muon': data['particle_masses_evolution'][7][-1],
|
| 33 |
+
'particle_mass_tau': data['particle_masses_evolution'][8][-1],
|
| 34 |
+
'particle_mass_photon': data['particle_masses_evolution'][9][-1],
|
| 35 |
+
'particle_speed': data['particle_speeds'][0][-1],
|
| 36 |
+
'particle_temperature': data['particle_temperatures'][0][-1],
|
| 37 |
+
})
|
| 38 |
+
|
| 39 |
+
df = pd.DataFrame(data_list)
|
| 40 |
+
|
| 41 |
+
# Scatter Plot: Tunneling Probability vs Various Particle Masses
|
| 42 |
+
plt.figure(figsize=(10, 8))
|
| 43 |
+
sns.scatterplot(x='tunneling_probability', y='particle_mass_up', data=df, label='Up Quark')
|
| 44 |
+
sns.scatterplot(x='tunneling_probability', y='particle_mass_down', data=df, label='Down Quark')
|
| 45 |
+
sns.scatterplot(x='tunneling_probability', y='particle_mass_charm', data=df, label='Charm Quark')
|
| 46 |
+
sns.scatterplot(x='tunneling_probability', y='particle_mass_strange', data=df, label='Strange Quark')
|
| 47 |
+
sns.scatterplot(x='tunneling_probability', y='particle_mass_top', data=df, label='Top Quark')
|
| 48 |
+
sns.scatterplot(x='tunneling_probability', y='particle_mass_bottom', data=df, label='Bottom Quark')
|
| 49 |
+
sns.scatterplot(x='tunneling_probability', y='particle_mass_electron', data=df, label='Electron')
|
| 50 |
+
sns.scatterplot(x='tunneling_probability', y='particle_mass_muon', data=df, label='Muon')
|
| 51 |
+
sns.scatterplot(x='tunneling_probability', y='particle_mass_tau', data=df, label='Tau')
|
| 52 |
+
sns.scatterplot(x='tunneling_probability', y='particle_mass_photon', data=df, label='Photon')
|
| 53 |
+
plt.title('Tunneling Probability vs Particle Masses')
|
| 54 |
+
plt.xlabel('Tunneling Probability')
|
| 55 |
+
plt.ylabel('Particle Mass (GeV)')
|
| 56 |
+
plt.legend()
|
| 57 |
+
plt.show()
|
| 58 |
+
|
| 59 |
+
# Heatmap: Correlation between Particle Masses
|
| 60 |
+
corr_matrix = df[['particle_mass_up', 'particle_mass_down', 'particle_mass_charm', 'particle_mass_strange', 'particle_mass_top', 'particle_mass_bottom', 'particle_mass_electron', 'particle_mass_muon', 'particle_mass_tau', 'particle_mass_photon']].corr()
|
| 61 |
+
plt.figure(figsize=(10, 8))
|
| 62 |
+
sns.heatmap(corr_matrix, annot=True, cmap='coolwarm', square=True)
|
| 63 |
+
plt.title('Correlation between Particle Masses')
|
| 64 |
+
plt.show()
|
| 65 |
+
|
| 66 |
+
# PCA
|
| 67 |
+
features = ['particle_mass_up', 'particle_mass_down', 'particle_mass_charm', 'particle_mass_strange', 'particle_mass_top', 'particle_mass_bottom', 'particle_mass_electron', 'particle_mass_muon', 'particle_mass_tau', 'particle_mass_photon', 'particle_speed', 'particle_temperature']
|
| 68 |
+
X = df[features]
|
| 69 |
+
pca = PCA(n_components=2)
|
| 70 |
+
principal_components = pca.fit_transform(X)
|
| 71 |
+
pca_df = pd.DataFrame(data=principal_components, columns=['PC1', 'PC2'])
|
| 72 |
+
|
| 73 |
+
# PCA Plot
|
| 74 |
+
plt.figure(figsize=(8, 6))
|
| 75 |
+
sns.scatterplot(x='PC1', y='PC2', data=pca_df, hue=df['tunneling_probability'], palette='viridis')
|
| 76 |
+
plt.title('PCA of Particle Properties')
|
| 77 |
+
plt.xlabel('Principal Component 1')
|
| 78 |
+
plt.ylabel('Principal Component 2')
|
| 79 |
+
plt.show()
|
pi.py
ADDED
|
@@ -0,0 +1,35 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import numpy as np
|
| 2 |
+
import matplotlib.pyplot as plt
|
| 3 |
+
|
| 4 |
+
# Constants
|
| 5 |
+
num_samples = 1000000 # Number of random samples
|
| 6 |
+
radius = 1.0 # Radius of the circle
|
| 7 |
+
|
| 8 |
+
# Generate random points in the unit square [0, 1] x [0, 1]
|
| 9 |
+
x = np.random.uniform(-radius, radius, num_samples)
|
| 10 |
+
y = np.random.uniform(-radius, radius, num_samples)
|
| 11 |
+
|
| 12 |
+
# Count how many points fall inside the quarter circle
|
| 13 |
+
inside_circle = np.sum(x**2 + y**2 <= radius**2)
|
| 14 |
+
|
| 15 |
+
# Estimate pi using the ratio of points inside the circle to total points
|
| 16 |
+
pi_estimate = (inside_circle / num_samples) * 4
|
| 17 |
+
print(f"Estimated value of pi with {num_samples} samples: {pi_estimate}")
|
| 18 |
+
|
| 19 |
+
# Optional: Visualize the points
|
| 20 |
+
def plot_simulation(x, y):
|
| 21 |
+
plt.figure(figsize=(8, 8))
|
| 22 |
+
plt.scatter(x[x**2 + y**2 <= radius**2], y[x**2 + y**2 <= radius**2], color='blue', s=1) # Points inside the circle
|
| 23 |
+
plt.scatter(x[x**2 + y**2 > radius**2], y[x**2 + y**2 > radius**2], color='red', s=1) # Points outside the circle
|
| 24 |
+
plt.xlim(-1.5, 1.5)
|
| 25 |
+
plt.ylim(-1.5, 1.5)
|
| 26 |
+
plt.title('Monte Carlo Simulation of Pi')
|
| 27 |
+
plt.gca().set_aspect('equal', adjustable='box')
|
| 28 |
+
plt.axhline(0, color='black', lw=0.5)
|
| 29 |
+
plt.axvline(0, color='black', lw=0.5)
|
| 30 |
+
plt.grid()
|
| 31 |
+
plt.show()
|
| 32 |
+
|
| 33 |
+
# Uncomment the line below to visualize the simulation
|
| 34 |
+
# plot_simulation(x, y)
|
| 35 |
+
|
pi1.py
ADDED
|
@@ -0,0 +1,43 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import numpy as np
|
| 2 |
+
import matplotlib.pyplot as plt
|
| 3 |
+
|
| 4 |
+
# Constants
|
| 5 |
+
num_particles = 1000000 # Increase the number of particles for better accuracy
|
| 6 |
+
radius = 1.0 # Radius of the circle
|
| 7 |
+
|
| 8 |
+
# Generate random points in the unit square [-1, 1] x [-1, 1]
|
| 9 |
+
x_positions = np.random.uniform(-radius, radius, num_particles)
|
| 10 |
+
y_positions = np.random.uniform(-radius, radius, num_particles)
|
| 11 |
+
|
| 12 |
+
# Function to estimate pi based on particle positions
|
| 13 |
+
def estimate_pi_from_particles(x_positions, y_positions):
|
| 14 |
+
inside_circle = np.sum(x_positions**2 + y_positions**2 <= radius**2)
|
| 15 |
+
total_particles = len(x_positions)
|
| 16 |
+
pi_estimate = (inside_circle / total_particles) * 4 # Area ratio method
|
| 17 |
+
return pi_estimate
|
| 18 |
+
|
| 19 |
+
# Estimate pi
|
| 20 |
+
pi_estimate = estimate_pi_from_particles(x_positions, y_positions)
|
| 21 |
+
print(f"Estimated value of pi based on particle positions: {pi_estimate}")
|
| 22 |
+
|
| 23 |
+
# Optional: Visualize the particles
|
| 24 |
+
def plot_particles(x_positions, y_positions):
|
| 25 |
+
plt.figure(figsize=(8, 8))
|
| 26 |
+
plt.scatter(x_positions[x_positions**2 + y_positions**2 <= radius**2],
|
| 27 |
+
y_positions[x_positions**2 + y_positions**2 <= radius**2],
|
| 28 |
+
color='blue', s=1) # Points inside the circle
|
| 29 |
+
plt.scatter(x_positions[x_positions**2 + y_positions**2 > radius**2],
|
| 30 |
+
y_positions[x_positions**2 + y_positions**2 > radius**2],
|
| 31 |
+
color='red', s=1) # Points outside the circle
|
| 32 |
+
plt.xlim(-1.5, 1.5)
|
| 33 |
+
plt.ylim(-1.5, 1.5)
|
| 34 |
+
plt.title('Monte Carlo Simulation of Pi')
|
| 35 |
+
plt.gca().set_aspect('equal', adjustable='box')
|
| 36 |
+
plt.axhline(0, color='black', lw=0.5)
|
| 37 |
+
plt.axvline(0, color='black', lw=0.5)
|
| 38 |
+
plt.grid()
|
| 39 |
+
plt.show()
|
| 40 |
+
|
| 41 |
+
# Uncomment the line below to visualize the particles
|
| 42 |
+
# plot_particles(x_positions, y_positions)
|
| 43 |
+
|
pi2.py
ADDED
|
@@ -0,0 +1,53 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import decimal
|
| 2 |
+
from decimal import Decimal, getcontext
|
| 3 |
+
|
| 4 |
+
# Set the precision
|
| 5 |
+
getcontext().prec = 110
|
| 6 |
+
|
| 7 |
+
# Constants
|
| 8 |
+
c = 299792458 # Speed of light in m/s
|
| 9 |
+
h = Decimal('6.62607015e-34') # Planck constant in J*s
|
| 10 |
+
k_B = Decimal('1.38e-23') # Boltzmann constant in J/K
|
| 11 |
+
TSR = Decimal(c**2) / k_B # Temperature to Speed Ratio in K*m/s
|
| 12 |
+
Q = Decimal('2') ** (Decimal('1') / Decimal('12')) # Fractal structure parameter
|
| 13 |
+
|
| 14 |
+
def chudnovsky_pi(n_terms):
|
| 15 |
+
C = Decimal(426880) * Decimal(10005).sqrt()
|
| 16 |
+
K = Decimal(6)
|
| 17 |
+
M = Decimal(1)
|
| 18 |
+
X = Decimal(1)
|
| 19 |
+
L = Decimal(13591409)
|
| 20 |
+
S = Decimal(0) # Initialize S to 0
|
| 21 |
+
for i in range(1, n_terms + 1): # Change to n_terms + 1 to avoid i = 0
|
| 22 |
+
if i == 1: # Handle the first iteration separately
|
| 23 |
+
M = Decimal(1) # Set M to 1 for the first iteration
|
| 24 |
+
else:
|
| 25 |
+
divisor = Decimal((i-1)**3)
|
| 26 |
+
if divisor == Decimal(0): # Check for zero divisor
|
| 27 |
+
divisor = Decimal(1) # Set divisor to 1 to avoid division by zero
|
| 28 |
+
M = (K**3 - Decimal(16)*K) * M // divisor
|
| 29 |
+
L += Decimal(545140134)
|
| 30 |
+
X *= Decimal(-262537412640768000)
|
| 31 |
+
term = Decimal(M * L) / X
|
| 32 |
+
# Apply fractal Q to the term
|
| 33 |
+
term *= Q ** (Decimal(i) / Decimal(n_terms))
|
| 34 |
+
# Apply TSR and quantum fluctuations conservatively
|
| 35 |
+
if term < Decimal('1e-15'):
|
| 36 |
+
TSR_rel = TSR
|
| 37 |
+
ΔTSR_q = Decimal('0')
|
| 38 |
+
else:
|
| 39 |
+
TSR_rel = TSR / Decimal((1 - (term**2 / Decimal(c**2))).sqrt())
|
| 40 |
+
ΔTSR_q = h * term
|
| 41 |
+
S += term * TSR_rel + ΔTSR_q
|
| 42 |
+
K += Decimal(12)
|
| 43 |
+
pi = C / S
|
| 44 |
+
return +pi
|
| 45 |
+
|
| 46 |
+
# Example usage
|
| 47 |
+
pi = chudnovsky_pi(100)
|
| 48 |
+
print(f"π ≈ {pi}")
|
| 49 |
+
|
| 50 |
+
# Save results to a JSON file
|
| 51 |
+
import json
|
| 52 |
+
with open('pi_simulation_results.json', 'w') as f:
|
| 53 |
+
json.dump({"pi_approx": str(pi)}, f)
|
pi3.py
ADDED
|
@@ -0,0 +1,148 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import numpy as np
|
| 2 |
+
import pandas as pd
|
| 3 |
+
import json
|
| 4 |
+
import os
|
| 5 |
+
|
| 6 |
+
# Constants
|
| 7 |
+
c = 299792458 # Speed of light in m/s
|
| 8 |
+
E_mc2 = c**2 # Mass-energy equivalence in J/kg
|
| 9 |
+
TSR = E_mc2 / (1.38e-23) # Temperature to Speed Ratio in K/m/s
|
| 10 |
+
alpha = 1.0 # Proportional constant for TSR
|
| 11 |
+
Q = 2 ** (1 / 12) # Fractal structure parameter
|
| 12 |
+
dark_energy_density = 5.96e-27 # Density of dark energy in kg/m^3
|
| 13 |
+
dark_matter_density = 2.25e-27 # Density of dark matter in kg/m^3
|
| 14 |
+
collision_distance = 1e-10 # Distance for collision detection
|
| 15 |
+
Hubble_constant = 70.0 # km/s/Mpc (approximation)
|
| 16 |
+
Hubble_constant_SI = Hubble_constant * 1000 / 3.086e22 # Convert to SI units (s^-1)
|
| 17 |
+
|
| 18 |
+
# Initial conditions
|
| 19 |
+
temperature_initial = 1.0 # Planck temperature in K
|
| 20 |
+
particle_density_initial = 5.16e96 # Planck density in kg/m^3
|
| 21 |
+
particle_speed_initial = TSR * temperature_initial # Initial speed based on TSR
|
| 22 |
+
|
| 23 |
+
# Simulation time
|
| 24 |
+
t_planck = 5.39e-44 # Planck time in s
|
| 25 |
+
t_simulation = t_planck * 1e5 # Shorter timescale for simulation
|
| 26 |
+
|
| 27 |
+
# Quark masses (in GeV) - used for initial mass values and comparison
|
| 28 |
+
quark_masses = {
|
| 29 |
+
"up": 2.3e-3,
|
| 30 |
+
"down": 4.8e-3,
|
| 31 |
+
"charm": 1.28,
|
| 32 |
+
"strange": 0.095,
|
| 33 |
+
"top": 173.0,
|
| 34 |
+
"bottom": 4.18,
|
| 35 |
+
"electron": 5.11e-4,
|
| 36 |
+
"muon": 1.05e-1,
|
| 37 |
+
"tau": 1.78,
|
| 38 |
+
"photon": 0,
|
| 39 |
+
}
|
| 40 |
+
|
| 41 |
+
# Conversion factor from GeV to J
|
| 42 |
+
GeV_to_J = 1.60217662e-10
|
| 43 |
+
|
| 44 |
+
# Simulation setup
|
| 45 |
+
num_steps = int(t_simulation / t_planck)
|
| 46 |
+
|
| 47 |
+
# Tunneling probabilities to investigate
|
| 48 |
+
tunneling_probabilities = np.arange(0.00000000001, 0.00000000010, 0.00000000001 ) # Exclude 1.0
|
| 49 |
+
|
| 50 |
+
# Create a directory to store the data
|
| 51 |
+
data_dir = "big_bang_simulation_data"
|
| 52 |
+
os.makedirs(data_dir, exist_ok=True)
|
| 53 |
+
|
| 54 |
+
# Functions to incorporate relativistic effects and collisions
|
| 55 |
+
def relativistic_energy(particle_speed, particle_mass):
|
| 56 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 57 |
+
return particle_mass * c**2 / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 58 |
+
|
| 59 |
+
def relativistic_momentum(particle_speed, particle_mass):
|
| 60 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 61 |
+
return particle_mass * particle_speed / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 62 |
+
|
| 63 |
+
def update_speed(current_speed, current_temperature, particle_mass):
|
| 64 |
+
"""Update the speed of a particle based on temperature and mass."""
|
| 65 |
+
return TSR * current_temperature # Update speed using TSR
|
| 66 |
+
|
| 67 |
+
def check_collision(particle_speeds, collision_distance):
|
| 68 |
+
epsilon = 1e-15 # A small value to avoid invalid subtraction
|
| 69 |
+
for j in range(len(particle_speeds)):
|
| 70 |
+
for k in range(j+1, len(particle_speeds)):
|
| 71 |
+
if np.abs(particle_speeds[j] - particle_speeds[k]) < collision_distance + epsilon:
|
| 72 |
+
return True, j, k
|
| 73 |
+
return False, -1, -1
|
| 74 |
+
|
| 75 |
+
def handle_collision(particle_speeds, particle_masses, idx1, idx2):
|
| 76 |
+
"""Handle a collision between two particles."""
|
| 77 |
+
p1 = relativistic_momentum(particle_speeds[idx1], particle_masses[idx1])
|
| 78 |
+
p2 = relativistic_momentum(particle_speeds[idx2], particle_masses[idx2])
|
| 79 |
+
|
| 80 |
+
# Calculate velocities after collision using conservation of momentum
|
| 81 |
+
total_momentum = p1 + p2
|
| 82 |
+
total_mass = particle_masses[idx1] + particle_masses[idx2]
|
| 83 |
+
v1_new = (total_momentum / total_mass) * (particle_masses[idx1] / total_mass)
|
| 84 |
+
v2_new = (total_momentum / total_mass) * (particle_masses[idx2] / total_mass)
|
| 85 |
+
|
| 86 |
+
particle_speeds[idx1], particle_speeds[idx2] = v1_new, v2_new
|
| 87 |
+
|
| 88 |
+
#...
|
| 89 |
+
|
| 90 |
+
# Simulate the Big Bang with Dark Energy, Dark Matter, Tunneling, and Relativistic Effects
|
| 91 |
+
for tunneling_probability in tunneling_probabilities:
|
| 92 |
+
print(f"Simulating for tunneling probability: {tunneling_probability}")
|
| 93 |
+
|
| 94 |
+
# Initialize arrays for simulation
|
| 95 |
+
particle_speeds = np.zeros((len(quark_masses), num_steps)) # 2D array for speeds
|
| 96 |
+
particle_temperatures = np.zeros((len(quark_masses), num_steps)) # 2D array for temperatures
|
| 97 |
+
particle_masses_evolution = np.zeros((len(quark_masses), num_steps)) # 2D array for mass evolution
|
| 98 |
+
tunneling_steps = np.zeros((len(quark_masses), num_steps), dtype=bool) # 2D array for tunneling steps
|
| 99 |
+
|
| 100 |
+
# Create an array of masses for each quark
|
| 101 |
+
particle_masses = np.array([mass * GeV_to_J for mass in quark_masses.values()])
|
| 102 |
+
|
| 103 |
+
for j, (quark, mass) in enumerate(quark_masses.items()):
|
| 104 |
+
particle_masses_evolution[j, 0] = particle_masses[j] # Initialize mass
|
| 105 |
+
particle_speeds[j, 0] = particle_speed_initial # Initialize speed
|
| 106 |
+
particle_temperatures[j, 0] = temperature_initial # Initialize temperature
|
| 107 |
+
|
| 108 |
+
for i in range(1, num_steps):
|
| 109 |
+
# Update temperature based on expansion of the universe
|
| 110 |
+
particle_temperatures[j, i] = particle_temperatures[j, i-1] * (1 - Hubble_constant_SI * t_planck)
|
| 111 |
+
|
| 112 |
+
# Update speed using TSR
|
| 113 |
+
particle_speeds[j, i] = update_speed(particle_speeds[j, i-1], particle_temperatures[j, i], particle_masses[j])
|
| 114 |
+
|
| 115 |
+
# Apply tunneling effect
|
| 116 |
+
if np.random.rand() < tunneling_probability:
|
| 117 |
+
particle_speeds[j, i] = particle_speeds[j, 0]
|
| 118 |
+
tunneling_steps[j, i] = True
|
| 119 |
+
|
| 120 |
+
# Calculate entropy using von Neumann entropy formula
|
| 121 |
+
if particle_masses[j] == 0:
|
| 122 |
+
entropy = 0
|
| 123 |
+
else:
|
| 124 |
+
entropy = -particle_masses[j] * np.log1p(particle_masses[j])
|
| 125 |
+
|
| 126 |
+
# Update mass based on entropy
|
| 127 |
+
particle_masses_evolution[j, i] = particle_masses_evolution[j, i-1] + entropy / c**2
|
| 128 |
+
|
| 129 |
+
# Check for entanglement
|
| 130 |
+
if particle_speeds[j, i] == c and particle_temperatures[j, i] == 0:
|
| 131 |
+
print(f"Entanglement detected for particle {quark} at step {i}")
|
| 132 |
+
|
| 133 |
+
# Print calculated masses at the end of the simulation
|
| 134 |
+
print(f"Calculated masses at the end of the simulation using the von Neumann entropy (Tunneling Probability: {tunneling_probability}):")
|
| 135 |
+
for j, quark in enumerate(quark_masses.keys()):
|
| 136 |
+
print(f"{quark}: {particle_masses_evolution[j, -1] / GeV_to_J:.4e} GeV")
|
| 137 |
+
|
| 138 |
+
# Save data to JSON file
|
| 139 |
+
data_filename = os.path.join(data_dir, f"big_bang_simulation_data_{tunneling_probability:.2f}.json")
|
| 140 |
+
data = {
|
| 141 |
+
"tunneling_probability": tunneling_probability,
|
| 142 |
+
"particle_masses_evolution": particle_masses_evolution.tolist(),
|
| 143 |
+
"particle_speeds": particle_speeds.tolist(),
|
| 144 |
+
"particle_temperatures": particle_temperatures.tolist(),
|
| 145 |
+
"tunneling_steps": tunneling_steps.tolist()
|
| 146 |
+
}
|
| 147 |
+
with open(data_filename, "w") as f:
|
| 148 |
+
json.dump(data, f)
|
requirements.txt
ADDED
|
@@ -0,0 +1,9 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
streamlit==1.24.1
|
| 2 |
+
pandas>2.0
|
| 3 |
+
numpy<=1.25.1
|
| 4 |
+
plotly
|
| 5 |
+
cupy-cuda12x
|
| 6 |
+
matplotlib
|
| 7 |
+
scipy
|
| 8 |
+
tqdm
|
| 9 |
+
json
|
sim.py
ADDED
|
@@ -0,0 +1,391 @@
|
|
|
|
|
|
|
|
|
|
|
|
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|
|
|
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|
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|
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|
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|
| 1 |
+
import numpy as np
|
| 2 |
+
import matplotlib.pyplot as plt
|
| 3 |
+
from matplotlib.animation import FuncAnimation
|
| 4 |
+
from mpl_toolkits.mplot3d import Axes3D
|
| 5 |
+
import plotly.graph_objects as go
|
| 6 |
+
import pandas as pd
|
| 7 |
+
import json
|
| 8 |
+
import os
|
| 9 |
+
|
| 10 |
+
# Constants
|
| 11 |
+
c = 299792458 # Speed of light in m/s
|
| 12 |
+
E_mc2 = c**2 # Mass-energy equivalence in J/kg
|
| 13 |
+
TSR = E_mc2 / (1.38e-23) # Temperature to Speed Ratio in K/m/s
|
| 14 |
+
alpha = 1.0 # Proportional constant for TSR
|
| 15 |
+
Q = 2 ** (1 / 12) # Fractal structure parameter
|
| 16 |
+
dark_energy_density = 5.96e-27 # Density of dark energy in kg/m^3
|
| 17 |
+
dark_matter_density = 2.25e-27 # Density of dark matter in kg/m^3
|
| 18 |
+
collision_distance = 1e-10 # Distance for collision detection
|
| 19 |
+
Hubble_constant = 70.0 # km/s/Mpc (approximation)
|
| 20 |
+
Hubble_constant_SI = (
|
| 21 |
+
Hubble_constant * 1000 / 3.086e22
|
| 22 |
+
) # Hubble constant in SI units (s^-1)
|
| 23 |
+
|
| 24 |
+
# Initial conditions
|
| 25 |
+
temperature_initial = 1.42e32 # Planck temperature in K
|
| 26 |
+
particle_density_initial = 5.16e96 # Planck density in kg/m^3
|
| 27 |
+
particle_speed_initial = c # Initially at the speed of light
|
| 28 |
+
|
| 29 |
+
# Simulation time
|
| 30 |
+
t_planck = 5.39e-44 # Planck time in s
|
| 31 |
+
t_simulation = t_planck * 1e3 # Shorter timescale for simulation
|
| 32 |
+
|
| 33 |
+
# Quark masses (in GeV) - used for initial mass values and comparison
|
| 34 |
+
quark_masses = {
|
| 35 |
+
"up": 2.3e-3,
|
| 36 |
+
"down": 4.8e-3,
|
| 37 |
+
"charm": 1.28,
|
| 38 |
+
"strange": 0.095,
|
| 39 |
+
"top": 173.0,
|
| 40 |
+
"bottom": 4.18,
|
| 41 |
+
}
|
| 42 |
+
|
| 43 |
+
# Conversion factor from GeV to J
|
| 44 |
+
GeV_to_J = 1.60217662e-10
|
| 45 |
+
|
| 46 |
+
# Simulation setup
|
| 47 |
+
num_steps = int(t_simulation / t_planck)
|
| 48 |
+
|
| 49 |
+
# Tunneling probabilities to investigate
|
| 50 |
+
tunneling_probabilities = np.arange(0.1, 1.1, 0.1) # Exclude 1.0
|
| 51 |
+
|
| 52 |
+
# Create a directory to store the data
|
| 53 |
+
data_dir = "big_bang_simulation_data"
|
| 54 |
+
os.makedirs(data_dir, exist_ok=True)
|
| 55 |
+
|
| 56 |
+
# Functions to incorporate relativistic effects
|
| 57 |
+
def relativistic_energy(particle_speed, particle_mass):
|
| 58 |
+
if particle_speed >= c:
|
| 59 |
+
return np.inf
|
| 60 |
+
return particle_mass * c**2 / np.sqrt(max(1e-10, 1 - (particle_speed / c) ** 2))
|
| 61 |
+
|
| 62 |
+
|
| 63 |
+
def relativistic_momentum(particle_speed, particle_mass):
|
| 64 |
+
if particle_speed >= c:
|
| 65 |
+
return np.inf
|
| 66 |
+
return (
|
| 67 |
+
particle_mass
|
| 68 |
+
* particle_speed
|
| 69 |
+
/ np.sqrt(max(1e-10, 1 - (particle_speed / c) ** 2))
|
| 70 |
+
)
|
| 71 |
+
|
| 72 |
+
|
| 73 |
+
def update_speed(current_speed, current_temperature, particle_mass):
|
| 74 |
+
rel_momentum = relativistic_momentum(current_speed, particle_mass)
|
| 75 |
+
return c * np.sqrt(
|
| 76 |
+
max(1e-10, 1 - (rel_momentum / (rel_momentum + dark_energy_density)) ** 2)
|
| 77 |
+
)
|
| 78 |
+
|
| 79 |
+
|
| 80 |
+
# Simulate the Big Bang with Dark Energy, Dark Matter, Tunneling, and Relativistic Effects
|
| 81 |
+
correlation_matrices = [] # Initialize correlation_matrices list
|
| 82 |
+
|
| 83 |
+
for tunneling_probability in tunneling_probabilities:
|
| 84 |
+
print(f"Running simulation for tunneling probability: {tunneling_probability}")
|
| 85 |
+
|
| 86 |
+
# Initialize arrays for simulation
|
| 87 |
+
particle_speeds = np.zeros((len(quark_masses), num_steps)) # 2D array for speeds
|
| 88 |
+
particle_temperatures = np.zeros(
|
| 89 |
+
(len(quark_masses), num_steps)
|
| 90 |
+
) # 2D array for temperatures
|
| 91 |
+
particle_masses_evolution = np.zeros(
|
| 92 |
+
(len(quark_masses), num_steps)
|
| 93 |
+
) # 2D array for mass evolution
|
| 94 |
+
particle_positions = np.zeros(
|
| 95 |
+
(len(quark_masses), num_steps)
|
| 96 |
+
) # 2D array for positions
|
| 97 |
+
tunneling_steps = np.zeros(
|
| 98 |
+
(len(quark_masses), num_steps), dtype=bool
|
| 99 |
+
) # 2D array for tunneling steps
|
| 100 |
+
|
| 101 |
+
# Create an array of masses for each quark
|
| 102 |
+
particle_masses = np.array([mass * GeV_to_J for mass in quark_masses.values()])
|
| 103 |
+
|
| 104 |
+
for j, (quark, mass) in enumerate(quark_masses.items()):
|
| 105 |
+
particle_masses_evolution[j, 0] = particle_masses[j] # Initialize mass
|
| 106 |
+
particle_positions[j, 0] = 0 # Initialize position
|
| 107 |
+
|
| 108 |
+
for i in range(1, num_steps):
|
| 109 |
+
particle_speeds[j, i] = update_speed(
|
| 110 |
+
particle_speeds[j, i - 1],
|
| 111 |
+
particle_temperatures[j, i - 1],
|
| 112 |
+
particle_masses[j],
|
| 113 |
+
)
|
| 114 |
+
particle_positions[j, i] = (
|
| 115 |
+
particle_positions[j, i - 1] + particle_speeds[j, i] * t_planck
|
| 116 |
+
) # Update position
|
| 117 |
+
|
| 118 |
+
value = (
|
| 119 |
+
1
|
| 120 |
+
- (particle_speeds[j, i] / (TSR * temperature_initial))
|
| 121 |
+
+ dark_matter_density
|
| 122 |
+
)
|
| 123 |
+
|
| 124 |
+
if np.random.rand() < tunneling_probability:
|
| 125 |
+
particle_speeds[j, i] = particle_speeds[j, 0] # Tunneling effect
|
| 126 |
+
tunneling_steps[j, i] = True # Mark tunneling step
|
| 127 |
+
|
| 128 |
+
if value < 0:
|
| 129 |
+
value = 0
|
| 130 |
+
|
| 131 |
+
particle_temperatures[j, i] = (
|
| 132 |
+
alpha * particle_speeds[j, i] ** 2
|
| 133 |
+
) # Apply TSR equation
|
| 134 |
+
|
| 135 |
+
# Update mass based on energy conversion
|
| 136 |
+
speed_squared_diff = (
|
| 137 |
+
particle_speeds[j, i] ** 2 - particle_speeds[j, i - 1] ** 2
|
| 138 |
+
)
|
| 139 |
+
|
| 140 |
+
# Avoid division by zero (if speed doesn't change, mass doesn't change)
|
| 141 |
+
if speed_squared_diff == 0:
|
| 142 |
+
particle_masses_evolution[j, i] = particle_masses_evolution[j, i - 1]
|
| 143 |
+
else:
|
| 144 |
+
# Calculate the change in relativistic energy
|
| 145 |
+
energy_diff = relativistic_energy(
|
| 146 |
+
particle_speeds[j, i], particle_masses[j]
|
| 147 |
+
) - relativistic_energy(particle_speeds[j, i - 1], particle_masses[j])
|
| 148 |
+
|
| 149 |
+
# Avoid NaN by checking if energy_diff is practically zero
|
| 150 |
+
if abs(energy_diff) < 1e-15: # Adjust the tolerance as needed
|
| 151 |
+
particle_masses_evolution[j, i] = particle_masses_evolution[
|
| 152 |
+
j, i - 1
|
| 153 |
+
]
|
| 154 |
+
else:
|
| 155 |
+
# Update mass based on energy difference
|
| 156 |
+
new_mass = (
|
| 157 |
+
particle_masses_evolution[j, i - 1] + energy_diff / c**2
|
| 158 |
+
)
|
| 159 |
+
if np.isfinite(new_mass): # Check if the new mass is finite
|
| 160 |
+
particle_masses_evolution[j, i] = new_mass
|
| 161 |
+
else:
|
| 162 |
+
particle_masses_evolution[j, i] = particle_masses_evolution[
|
| 163 |
+
j, i - 1
|
| 164 |
+
]
|
| 165 |
+
|
| 166 |
+
# Collision detection and resolution
|
| 167 |
+
for k in range(j + 1, len(quark_masses)):
|
| 168 |
+
if (
|
| 169 |
+
abs(particle_positions[j, i] - particle_positions[k, i])
|
| 170 |
+
< collision_distance
|
| 171 |
+
):
|
| 172 |
+
# Resolve collision (simplified example)
|
| 173 |
+
# Calculate relative speed before the collision
|
| 174 |
+
v_rel = particle_speeds[j, i] - particle_speeds[k, i]
|
| 175 |
+
|
| 176 |
+
# Calculate the new speeds after the collision
|
| 177 |
+
particle_speeds[j, i] = (
|
| 178 |
+
particle_speeds[j, i]
|
| 179 |
+
* (particle_masses[j] - particle_masses[k])
|
| 180 |
+
+ 2 * particle_masses[k] * particle_speeds[k, i]
|
| 181 |
+
) / (particle_masses[j] + particle_masses[k])
|
| 182 |
+
particle_speeds[k, i] = (
|
| 183 |
+
particle_speeds[k, i]
|
| 184 |
+
* (particle_masses[k] - particle_masses[j])
|
| 185 |
+
+ 2 * particle_masses[j] * particle_speeds[j, i]
|
| 186 |
+
) / (particle_masses[j] + particle_masses[k])
|
| 187 |
+
|
| 188 |
+
# Limit speed after collision
|
| 189 |
+
max_speed = c * 0.99 # Adjust the maximum speed as needed
|
| 190 |
+
particle_speeds[j, i] = np.clip(particle_speeds[j, i], 0, max_speed)
|
| 191 |
+
particle_speeds[k, i] = np.clip(particle_speeds[k, i], 0, max_speed)
|
| 192 |
+
|
| 193 |
+
# Update temperatures based on TSR
|
| 194 |
+
particle_temperatures[j, i] = alpha * particle_speeds[j, i] ** 2
|
| 195 |
+
particle_temperatures[k, i] = alpha * particle_speeds[k, i] ** 2
|
| 196 |
+
|
| 197 |
+
# Apply expansion of the universe (redshift)
|
| 198 |
+
particle_speeds[j, i] *= 1 - Hubble_constant_SI * t_planck
|
| 199 |
+
|
| 200 |
+
# Apply expansion of the universe (cooling)
|
| 201 |
+
particle_temperatures[j, i] *= 1 - Hubble_constant_SI * t_planck
|
| 202 |
+
|
| 203 |
+
# Debugging output
|
| 204 |
+
if np.isnan(particle_speeds[j, i]) or np.isnan(particle_temperatures[j, i]):
|
| 205 |
+
print(f"NaN detected at step {i} for quark {quark}")
|
| 206 |
+
print(f"Previous speed: {particle_speeds[j, i - 1]}")
|
| 207 |
+
print(f"Previous temperature: {particle_temperatures[j, i - 1]}")
|
| 208 |
+
print(f"Current speed: {particle_speeds[j, i]}")
|
| 209 |
+
print(f"Current temperature: {particle_temperatures[j, i]}")
|
| 210 |
+
break
|
| 211 |
+
|
| 212 |
+
# Cap speed to avoid unphysical values
|
| 213 |
+
particle_speeds[j] = np.clip(particle_speeds[j], 0, c)
|
| 214 |
+
|
| 215 |
+
# --- Plotly Interactive Visualization (3D) ---
|
| 216 |
+
# Create the 3D scatter plot using Plotly
|
| 217 |
+
fig = go.Figure(
|
| 218 |
+
data=[
|
| 219 |
+
go.Scatter3d(
|
| 220 |
+
x=particle_speeds[j],
|
| 221 |
+
y=particle_temperatures[j],
|
| 222 |
+
z=np.arange(num_steps),
|
| 223 |
+
mode="lines+markers",
|
| 224 |
+
name=quark.capitalize(),
|
| 225 |
+
)
|
| 226 |
+
for j, quark in enumerate(quark_masses.keys())
|
| 227 |
+
]
|
| 228 |
+
)
|
| 229 |
+
fig.update_layout(
|
| 230 |
+
title=f"Big Bang Simulation: Temperature vs. Speed (Tunneling Probability: {tunneling_probability})",
|
| 231 |
+
autosize=False,
|
| 232 |
+
width=800,
|
| 233 |
+
height=600,
|
| 234 |
+
margin=dict(l=65, r=50, b=65, t=90),
|
| 235 |
+
)
|
| 236 |
+
fig.show()
|
| 237 |
+
|
| 238 |
+
# --- Matplotlib Animation (3D) ---
|
| 239 |
+
fig = plt.figure()
|
| 240 |
+
ax = fig.add_subplot(111, projection="3d")
|
| 241 |
+
(line,) = ax.plot([], [], [], "b-")
|
| 242 |
+
|
| 243 |
+
# Set axis limits
|
| 244 |
+
ax.set_xlim(min(particle_speeds.flatten()), max(particle_speeds.flatten()))
|
| 245 |
+
ax.set_ylim(
|
| 246 |
+
min(particle_temperatures.flatten()), max(particle_temperatures.flatten())
|
| 247 |
+
)
|
| 248 |
+
ax.set_zlim(0, num_steps)
|
| 249 |
+
|
| 250 |
+
ax.set_xlabel("Particle Speed")
|
| 251 |
+
ax.set_ylabel("Particle Temperature")
|
| 252 |
+
ax.set_zlabel("Time")
|
| 253 |
+
ax.set_title(
|
| 254 |
+
f"Big Bang Simulation Animation (Tunneling Probability: {tunneling_probability})"
|
| 255 |
+
)
|
| 256 |
+
|
| 257 |
+
def init():
|
| 258 |
+
line.set_data([], [])
|
| 259 |
+
line.set_3d_properties([])
|
| 260 |
+
return (line,)
|
| 261 |
+
|
| 262 |
+
def update(frame):
|
| 263 |
+
line.set_data(
|
| 264 |
+
particle_speeds[:, :frame].flatten(),
|
| 265 |
+
particle_temperatures[:, :frame].flatten(),
|
| 266 |
+
)
|
| 267 |
+
line.set_3d_properties(np.tile(np.arange(frame), len(quark_masses)))
|
| 268 |
+
return (line,)
|
| 269 |
+
|
| 270 |
+
ani = FuncAnimation(fig, update, frames=num_steps, init_func=init, blit=True)
|
| 271 |
+
ani.save(f"big_bang_simulation_3d_{tunneling_probability}.gif", writer="pillow")
|
| 272 |
+
plt.show()
|
| 273 |
+
|
| 274 |
+
# --- Plotly Mass Evolution (3D) ---
|
| 275 |
+
X, Y = np.meshgrid(
|
| 276 |
+
particle_speeds[0], np.arange(num_steps)
|
| 277 |
+
) # Create 2D meshgrid for x and y
|
| 278 |
+
fig = go.Figure(
|
| 279 |
+
data=[
|
| 280 |
+
go.Surface(
|
| 281 |
+
z=particle_masses_evolution[j],
|
| 282 |
+
x=X,
|
| 283 |
+
y=Y,
|
| 284 |
+
colorscale="Viridis",
|
| 285 |
+
name=quark.capitalize(),
|
| 286 |
+
)
|
| 287 |
+
for j, quark in enumerate(quark_masses.keys())
|
| 288 |
+
]
|
| 289 |
+
)
|
| 290 |
+
fig.update_layout(
|
| 291 |
+
title=f"Big Bang Simulation: Mass Evolution (Tunneling Probability: {tunneling_probability})",
|
| 292 |
+
autosize=False,
|
| 293 |
+
width=800,
|
| 294 |
+
height=600,
|
| 295 |
+
margin=dict(l=65, r=50, b=65, t=90),
|
| 296 |
+
)
|
| 297 |
+
fig.show()
|
| 298 |
+
|
| 299 |
+
# --- Plotly Tunneling Effect (3D) ---
|
| 300 |
+
X, Y = np.meshgrid(
|
| 301 |
+
particle_speeds[0], np.arange(num_steps)
|
| 302 |
+
) # Create 2D meshgrid for x and y
|
| 303 |
+
fig = go.Figure(
|
| 304 |
+
data=[
|
| 305 |
+
go.Surface(
|
| 306 |
+
z=tunneling_steps[j],
|
| 307 |
+
x=X,
|
| 308 |
+
y=Y,
|
| 309 |
+
colorscale="Blues",
|
| 310 |
+
name=quark.capitalize(),
|
| 311 |
+
)
|
| 312 |
+
for j, quark in enumerate(quark_masses.keys())
|
| 313 |
+
]
|
| 314 |
+
)
|
| 315 |
+
fig.update_layout(
|
| 316 |
+
title=f"Big Bang Simulation: Tunneling Effect (Tunneling Probability: {tunneling_probability})",
|
| 317 |
+
autosize=False,
|
| 318 |
+
width=800,
|
| 319 |
+
height=600,
|
| 320 |
+
margin=dict(l=65, r=50, b=65, t=90),
|
| 321 |
+
)
|
| 322 |
+
fig.show()
|
| 323 |
+
|
| 324 |
+
# --- Correlation Analysis ---
|
| 325 |
+
df = pd.DataFrame(
|
| 326 |
+
{
|
| 327 |
+
"Speed": particle_speeds.flatten(),
|
| 328 |
+
"Temperature": particle_temperatures.flatten(),
|
| 329 |
+
"Mass": particle_masses_evolution.flatten(),
|
| 330 |
+
"Tunneling": tunneling_steps.flatten(),
|
| 331 |
+
}
|
| 332 |
+
)
|
| 333 |
+
|
| 334 |
+
correlation_matrix = df.corr()
|
| 335 |
+
correlation_matrices.append(correlation_matrix)
|
| 336 |
+
|
| 337 |
+
print("Correlation Matrix:")
|
| 338 |
+
print(correlation_matrix)
|
| 339 |
+
|
| 340 |
+
# Print calculated masses at the end of the simulation
|
| 341 |
+
print(
|
| 342 |
+
f"Calculated masses at the end of the simulation (Tunneling Probability: {tunneling_probability}):"
|
| 343 |
+
)
|
| 344 |
+
for j, quark in enumerate(quark_masses.keys()):
|
| 345 |
+
print(f"{quark}: {particle_masses_evolution[j, -1] / GeV_to_J:.4e} GeV")
|
| 346 |
+
print("Real masses:")
|
| 347 |
+
for quark, mass in quark_masses.items():
|
| 348 |
+
print(f"{quark}: {mass:.4e} GeV")
|
| 349 |
+
|
| 350 |
+
# Save data to JSON file
|
| 351 |
+
data_filename = os.path.join(
|
| 352 |
+
data_dir, f"big_bang_simulation_data_{tunneling_probability:.1f}.json"
|
| 353 |
+
)
|
| 354 |
+
data = {
|
| 355 |
+
"tunneling_probability": tunneling_probability,
|
| 356 |
+
"particle_speeds": particle_speeds.tolist(),
|
| 357 |
+
"particle_temperatures": particle_temperatures.tolist(),
|
| 358 |
+
"particle_masses_evolution": particle_masses_evolution.tolist(),
|
| 359 |
+
"tunneling_steps": tunneling_steps.tolist(),
|
| 360 |
+
"correlation_matrix": correlation_matrix.values.tolist(), # Use values.tolist() to convert DataFrame to list
|
| 361 |
+
}
|
| 362 |
+
with open(data_filename, "w") as f:
|
| 363 |
+
json.dump(data, f)
|
| 364 |
+
|
| 365 |
+
correlation_matrices = []
|
| 366 |
+
for tunneling_probability in tunneling_probabilities:
|
| 367 |
+
#... (rest of the code remains the same)
|
| 368 |
+
correlation_matrix = df.corr()
|
| 369 |
+
if correlation_matrix.shape[0] == correlation_matrix.shape[1]:
|
| 370 |
+
correlation_matrices.append(correlation_matrix)
|
| 371 |
+
else:
|
| 372 |
+
print(f"Skipping correlation matrix for tunneling probability {tunneling_probability} because it is not a square matrix.")
|
| 373 |
+
|
| 374 |
+
# Flatten the correlation matrices
|
| 375 |
+
flat_correlation_matrices = []
|
| 376 |
+
for i, matrix in enumerate(correlation_matrices):
|
| 377 |
+
flattened = matrix.values.flatten()
|
| 378 |
+
flat_correlation_matrices.append(flattened)
|
| 379 |
+
|
| 380 |
+
# Convert to 2D array
|
| 381 |
+
flat_correlation_matrices = np.array(flat_correlation_matrices)
|
| 382 |
+
|
| 383 |
+
# Create DataFrame with appropriate column names
|
| 384 |
+
columns = [f"Corr_{i}_{j}" for i in range(flat_correlation_matrices.shape[1] // 4) for j in range(4)]
|
| 385 |
+
correlation_matrices_df = pd.DataFrame(flat_correlation_matrices, columns=columns, index=tunneling_probabilities)
|
| 386 |
+
|
| 387 |
+
# Print or save DataFrame
|
| 388 |
+
print("Correlation Matrices for Different Tunneling Probabilities:")
|
| 389 |
+
print(correlation_matrices_df)
|
| 390 |
+
|
| 391 |
+
|
sim10.py
ADDED
|
@@ -0,0 +1,198 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import numpy as np
|
| 2 |
+
import pandas as pd
|
| 3 |
+
import json
|
| 4 |
+
import os
|
| 5 |
+
|
| 6 |
+
# Constants
|
| 7 |
+
c = 299792458 # Speed of light in m/s
|
| 8 |
+
E_mc2 = c**2 # Mass-energy equivalence in J/kg
|
| 9 |
+
TSR = E_mc2 / (1.38e-23) # Temperature to Speed Ratio in K/m/s
|
| 10 |
+
alpha = 1.1056e-52 # Proportional constant for TSR
|
| 11 |
+
Q = 2 ** (1 / 12) # Fractal structure parameter
|
| 12 |
+
dark_energy_density = 5.96e-27 # Density of dark energy in kg/m^3
|
| 13 |
+
dark_matter_density = 2.25e-27 # Density of dark matter in kg/m^3
|
| 14 |
+
collision_distance = 1e-10 # Distance for collision detection
|
| 15 |
+
Hubble_constant = 70.0 # km/s/Mpc (approximation)
|
| 16 |
+
Hubble_constant_SI = (
|
| 17 |
+
Hubble_constant * 1000 / 3.086e22
|
| 18 |
+
) # Hubble constant in SI units (s^-1)
|
| 19 |
+
|
| 20 |
+
# Initial conditions
|
| 21 |
+
temperature_initial = 1.42e32 # Planck temperature in K
|
| 22 |
+
particle_density_initial = 5.16e96 # Planck density in kg/m^3
|
| 23 |
+
particle_speed_initial = c # Initially at the speed of light
|
| 24 |
+
|
| 25 |
+
# Simulation time
|
| 26 |
+
t_planck = 5.39e-44 # Planck time in s
|
| 27 |
+
t_simulation = t_planck * 1e5 # Shorter timescale for simulation
|
| 28 |
+
|
| 29 |
+
# Quark masses (in GeV) - used for initial mass values and comparison
|
| 30 |
+
quark_masses = {
|
| 31 |
+
"up": 2.3e-3,
|
| 32 |
+
"down": 4.8e-3,
|
| 33 |
+
"charm": 1.28,
|
| 34 |
+
"strange": 0.095,
|
| 35 |
+
"top": 173.0,
|
| 36 |
+
"bottom": 4.18,
|
| 37 |
+
"electron": 5.11e-4,
|
| 38 |
+
"muon": 1.05e-1,
|
| 39 |
+
"tau": 1.78,
|
| 40 |
+
"photon": 0,
|
| 41 |
+
}
|
| 42 |
+
|
| 43 |
+
# Conversion factor from GeV to J
|
| 44 |
+
GeV_to_J = 1.60217662e-10
|
| 45 |
+
|
| 46 |
+
# Simulation setup
|
| 47 |
+
num_steps = int(t_simulation / t_planck)
|
| 48 |
+
|
| 49 |
+
# Tunneling probabilities to investigate
|
| 50 |
+
tunneling_probabilities = np.arange(0.1, 4.1, 0.1) # Exclude 1.0
|
| 51 |
+
|
| 52 |
+
# Create a directory to store the data
|
| 53 |
+
data_dir = "big_bang_simulation_data"
|
| 54 |
+
os.makedirs(data_dir, exist_ok=True)
|
| 55 |
+
|
| 56 |
+
# Functions to incorporate relativistic effects and collisions
|
| 57 |
+
def relativistic_energy(particle_speed, particle_mass):
|
| 58 |
+
if particle_speed >= c:
|
| 59 |
+
return np.inf
|
| 60 |
+
return particle_mass * c**2 / np.sqrt(max(1e-10, 1 - (particle_speed / c) ** 2))
|
| 61 |
+
|
| 62 |
+
|
| 63 |
+
def relativistic_momentum(particle_speed, particle_mass):
|
| 64 |
+
if particle_speed >= c:
|
| 65 |
+
return np.inf
|
| 66 |
+
return (
|
| 67 |
+
particle_mass
|
| 68 |
+
* particle_speed
|
| 69 |
+
/ np.sqrt(max(1e-10, 1 - (particle_speed / c) ** 2))
|
| 70 |
+
)
|
| 71 |
+
|
| 72 |
+
|
| 73 |
+
def update_speed(current_speed, current_temperature, particle_mass):
|
| 74 |
+
rel_momentum = relativistic_momentum(current_speed, particle_mass)
|
| 75 |
+
return c * np.sqrt(
|
| 76 |
+
max(1e-10, 1 - (rel_momentum / (rel_momentum + dark_energy_density)) ** 2)
|
| 77 |
+
)
|
| 78 |
+
|
| 79 |
+
def check_collision(particle_speeds, collision_distance):
|
| 80 |
+
# Assuming 1D for simplicity. Expand for 3D if needed.
|
| 81 |
+
for j in range(len(particle_speeds)):
|
| 82 |
+
for k in range(j+1, len(particle_speeds)):
|
| 83 |
+
if np.abs(particle_speeds[j] - particle_speeds[k]) < collision_distance:
|
| 84 |
+
return True, j, k
|
| 85 |
+
return False, -1, -1
|
| 86 |
+
|
| 87 |
+
# Simulate the Big Bang with Dark Energy, Dark Matter, Tunneling, and Relativistic Effects
|
| 88 |
+
for tunneling_probability in tunneling_probabilities:
|
| 89 |
+
print(f"Simulating for tunneling probability: {tunneling_probability}")
|
| 90 |
+
|
| 91 |
+
# Initialize arrays for simulation
|
| 92 |
+
particle_speeds = np.zeros((len(quark_masses), num_steps)) # 2D array for speeds
|
| 93 |
+
particle_temperatures = np.zeros(
|
| 94 |
+
(len(quark_masses), num_steps)
|
| 95 |
+
) # 2D array for temperatures
|
| 96 |
+
particle_masses_evolution = np.zeros(
|
| 97 |
+
(len(quark_masses), num_steps)
|
| 98 |
+
) # 2D array for mass evolution
|
| 99 |
+
tunneling_steps = np.zeros(
|
| 100 |
+
(len(quark_masses), num_steps), dtype=bool
|
| 101 |
+
) # 2D array for tunneling steps
|
| 102 |
+
|
| 103 |
+
# Create an array of masses for each quark
|
| 104 |
+
particle_masses = np.array([mass * GeV_to_J for mass in quark_masses.values()])
|
| 105 |
+
|
| 106 |
+
for j, (quark, mass) in enumerate(quark_masses.items()):
|
| 107 |
+
particle_masses_evolution[j, 0] = particle_masses[j] # Initialize mass
|
| 108 |
+
|
| 109 |
+
for i in range(1, num_steps):
|
| 110 |
+
particle_speeds[j, i] = update_speed(
|
| 111 |
+
particle_speeds[j, i - 1],
|
| 112 |
+
particle_temperatures[j, i - 1],
|
| 113 |
+
particle_masses[j],
|
| 114 |
+
)
|
| 115 |
+
|
| 116 |
+
value = (
|
| 117 |
+
1
|
| 118 |
+
- (particle_speeds[j, i] / (TSR * temperature_initial))
|
| 119 |
+
+ dark_matter_density
|
| 120 |
+
)
|
| 121 |
+
|
| 122 |
+
if np.random.rand() < tunneling_probability:
|
| 123 |
+
particle_speeds[j, i] = particle_speeds[j, 0] # Tunneling effect
|
| 124 |
+
tunneling_steps[j, i] = True # Mark tunneling step
|
| 125 |
+
|
| 126 |
+
if value < 0:
|
| 127 |
+
value = 0
|
| 128 |
+
|
| 129 |
+
particle_temperatures[j, i] = (
|
| 130 |
+
alpha * particle_speeds[j, i] ** 2
|
| 131 |
+
) # Apply TSR equation
|
| 132 |
+
|
| 133 |
+
# Update mass based on energy conversion
|
| 134 |
+
speed_squared_diff = (
|
| 135 |
+
particle_speeds[j, i] ** 2 - particle_speeds[j, i - 1] ** 2
|
| 136 |
+
)
|
| 137 |
+
|
| 138 |
+
# Avoid division by zero (if speed doesn't change, mass doesn't change)
|
| 139 |
+
if speed_squared_diff == 0:
|
| 140 |
+
particle_masses_evolution[j, i] = particle_masses_evolution[j, i - 1]
|
| 141 |
+
else:
|
| 142 |
+
# Calculate the change in relativistic energy
|
| 143 |
+
energy_diff = relativistic_energy(
|
| 144 |
+
particle_speeds[j, i], particle_masses[j]
|
| 145 |
+
) - relativistic_energy(particle_speeds[j, i - 1], particle_masses[j])
|
| 146 |
+
|
| 147 |
+
# Avoid NaN by checking if energy_diff is practically zero
|
| 148 |
+
if abs(energy_diff) < 1e-15: # Adjust the tolerance as needed
|
| 149 |
+
particle_masses_evolution[j, i] = particle_masses_evolution[
|
| 150 |
+
j, i - 1
|
| 151 |
+
]
|
| 152 |
+
else:
|
| 153 |
+
# Update mass based on energy difference
|
| 154 |
+
new_mass = (
|
| 155 |
+
particle_masses_evolution[j, i - 1] + energy_diff / c**2
|
| 156 |
+
)
|
| 157 |
+
if np.isfinite(new_mass): # Check if the new mass is finite
|
| 158 |
+
particle_masses_evolution[j, i] = new_mass
|
| 159 |
+
else:
|
| 160 |
+
particle_masses_evolution[j, i] = particle_masses_evolution[
|
| 161 |
+
j, i - 1
|
| 162 |
+
]
|
| 163 |
+
|
| 164 |
+
# Apply expansion of the universe (redshift)
|
| 165 |
+
particle_speeds[j, i] *= 1 - Hubble_constant_SI * t_planck
|
| 166 |
+
|
| 167 |
+
# Apply expansion of the universe (cooling)
|
| 168 |
+
particle_temperatures[j, i] *= 1 - Hubble_constant_SI * t_planck
|
| 169 |
+
|
| 170 |
+
# Check for collisions and handle them
|
| 171 |
+
collision, idx1, idx2 = check_collision(particle_speeds[:, i], collision_distance)
|
| 172 |
+
if collision:
|
| 173 |
+
# Simplified collision response: reverse speeds
|
| 174 |
+
particle_speeds[idx1, i], particle_speeds[idx2, i] = -particle_speeds[idx1, i], -particle_speeds[idx2, i]
|
| 175 |
+
|
| 176 |
+
# Print calculated masses at the end of the simulation
|
| 177 |
+
print(
|
| 178 |
+
f"Calculated masses at the end of the simulation (Tunneling Probability: {tunneling_probability}):"
|
| 179 |
+
)
|
| 180 |
+
for j, quark in enumerate(quark_masses.keys()):
|
| 181 |
+
print(
|
| 182 |
+
f"{quark}: {particle_masses_evolution[j, -1] / GeV_to_J:.4e} GeV"
|
| 183 |
+
)
|
| 184 |
+
|
| 185 |
+
# Save data to JSON file
|
| 186 |
+
data_filename = os.path.join(
|
| 187 |
+
data_dir, f"big_bang_simulation_data_{tunneling_probability:.2f}.json"
|
| 188 |
+
)
|
| 189 |
+
data = {
|
| 190 |
+
"tunneling_probability": tunneling_probability,
|
| 191 |
+
"particle_masses_evolution": particle_masses_evolution.tolist(),
|
| 192 |
+
"particle_speeds": particle_speeds.tolist(),
|
| 193 |
+
"particle_temperatures": particle_temperatures.tolist(),
|
| 194 |
+
"tunneling_steps": tunneling_steps.tolist()
|
| 195 |
+
}
|
| 196 |
+
with open(data_filename, "w") as f:
|
| 197 |
+
json.dump(data, f)
|
| 198 |
+
|
sim11.py
ADDED
|
@@ -0,0 +1,147 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
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|
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|
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|
|
|
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|
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|
|
|
|
|
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|
|
|
|
|
|
|
|
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|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import numpy as np
|
| 2 |
+
import pandas as pd
|
| 3 |
+
import json
|
| 4 |
+
import os
|
| 5 |
+
|
| 6 |
+
# Constants
|
| 7 |
+
c = 299792458 # Speed of light in m/s
|
| 8 |
+
E_mc2 = c**2 # Mass-energy equivalence in J/kg
|
| 9 |
+
TSR = E_mc2 / (1.38e-23) # Temperature to Speed Ratio in K/m/s
|
| 10 |
+
alpha = 1.0 # Proportional constant for TSR
|
| 11 |
+
Q = 2 ** (1 / 12) # Fractal structure parameter
|
| 12 |
+
dark_energy_density = 5.96e-27 # Density of dark energy in kg/m^3
|
| 13 |
+
dark_matter_density = 2.25e-27 # Density of dark matter in kg/m^3
|
| 14 |
+
collision_distance = 1e-10 # Distance for collision detection
|
| 15 |
+
Hubble_constant = 70.0 # km/s/Mpc (approximation)
|
| 16 |
+
Hubble_constant_SI = Hubble_constant * 1000 / 3.086e22 # Convert to SI units (s^-1)
|
| 17 |
+
|
| 18 |
+
# Initial conditions
|
| 19 |
+
temperature_initial = 1.0 # Planck temperature in K
|
| 20 |
+
particle_density_initial = 5.16e96 # Planck density in kg/m^3
|
| 21 |
+
particle_speed_initial = c # Initially at the speed of light
|
| 22 |
+
|
| 23 |
+
# Simulation time
|
| 24 |
+
t_planck = 5.39e-44 # Planck time in s
|
| 25 |
+
t_simulation = t_planck * 1e5 # Shorter timescale for simulation
|
| 26 |
+
|
| 27 |
+
# Quark masses (in GeV) - used for initial mass values and comparison
|
| 28 |
+
quark_masses = {
|
| 29 |
+
"up": 2.3e-3,
|
| 30 |
+
"down": 4.8e-3,
|
| 31 |
+
"charm": 1.28,
|
| 32 |
+
"strange": 0.095,
|
| 33 |
+
"top": 173.0,
|
| 34 |
+
"bottom": 4.18,
|
| 35 |
+
"electron": 5.11e-4,
|
| 36 |
+
"muon": 1.05e-1,
|
| 37 |
+
"tau": 1.78,
|
| 38 |
+
"photon": 0,
|
| 39 |
+
}
|
| 40 |
+
|
| 41 |
+
# Conversion factor from GeV to J
|
| 42 |
+
GeV_to_J = 1.60217662e-10
|
| 43 |
+
|
| 44 |
+
# Simulation setup
|
| 45 |
+
num_steps = int(t_simulation / t_planck)
|
| 46 |
+
|
| 47 |
+
# Tunneling probabilities to investigate
|
| 48 |
+
tunneling_probabilities = np.arange(99.1, 100.0, 0.1) # Exclude 1.0
|
| 49 |
+
|
| 50 |
+
# Create a directory to store the data
|
| 51 |
+
data_dir = "big_bang_simulation_data"
|
| 52 |
+
os.makedirs(data_dir, exist_ok=True)
|
| 53 |
+
|
| 54 |
+
# Functions to incorporate relativistic effects and collisions
|
| 55 |
+
def relativistic_energy(particle_speed, particle_mass):
|
| 56 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 57 |
+
return particle_mass * c**2 / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 58 |
+
|
| 59 |
+
def relativistic_momentum(particle_speed, particle_mass):
|
| 60 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 61 |
+
return particle_mass * particle_speed / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 62 |
+
|
| 63 |
+
def update_speed(current_speed, current_temperature, particle_mass):
|
| 64 |
+
"""Update the speed of a particle based on temperature and mass."""
|
| 65 |
+
rel_momentum = relativistic_momentum(current_speed, particle_mass)
|
| 66 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 67 |
+
return c * np.sqrt(1 - (rel_momentum / (rel_momentum + dark_energy_density + epsilon)) ** 2)
|
| 68 |
+
|
| 69 |
+
def check_collision(particle_speeds, collision_distance):
|
| 70 |
+
epsilon = 1e-15 # A small value to avoid invalid subtraction
|
| 71 |
+
for j in range(len(particle_speeds)):
|
| 72 |
+
for k in range(j+1, len(particle_speeds)):
|
| 73 |
+
if np.abs(particle_speeds[j] - particle_speeds[k]) < collision_distance + epsilon:
|
| 74 |
+
return True, j, k
|
| 75 |
+
return False, -1, -1
|
| 76 |
+
def handle_collision(particle_speeds, particle_masses, idx1, idx2):
|
| 77 |
+
"""Handle a collision between two particles."""
|
| 78 |
+
p1 = relativistic_momentum(particle_speeds[idx1], particle_masses[idx1])
|
| 79 |
+
p2 = relativistic_momentum(particle_speeds[idx2], particle_masses[idx2])
|
| 80 |
+
|
| 81 |
+
# Calculate velocities after collision using conservation of momentum
|
| 82 |
+
total_momentum = p1 + p2
|
| 83 |
+
total_mass = particle_masses[idx1] + particle_masses[idx2]
|
| 84 |
+
v1_new = (total_momentum / total_mass) * (particle_masses[idx1] / total_mass)
|
| 85 |
+
v2_new = (total_momentum / total_mass) * (particle_masses[idx2] / total_mass)
|
| 86 |
+
|
| 87 |
+
particle_speeds[idx1], particle_speeds[idx2] = v1_new, v2_new
|
| 88 |
+
|
| 89 |
+
# Simulate the Big Bang with Dark Energy, Dark Matter, Tunneling, and Relativistic Effects
|
| 90 |
+
for tunneling_probability in tunneling_probabilities:
|
| 91 |
+
print(f"Simulating for tunneling probability: {tunneling_probability}")
|
| 92 |
+
|
| 93 |
+
# Initialize arrays for simulation
|
| 94 |
+
particle_speeds = np.zeros((len(quark_masses), num_steps)) # 2D array for speeds
|
| 95 |
+
particle_temperatures = np.zeros((len(quark_masses), num_steps)) # 2D array for temperatures
|
| 96 |
+
particle_masses_evolution = np.zeros((len(quark_masses), num_steps)) # 2D array for mass evolution
|
| 97 |
+
tunneling_steps = np.zeros((len(quark_masses), num_steps), dtype=bool) # 2D array for tunneling steps
|
| 98 |
+
|
| 99 |
+
# Create an array of masses for each quark
|
| 100 |
+
particle_masses = np.array([mass * GeV_to_J for mass in quark_masses.values()])
|
| 101 |
+
|
| 102 |
+
for j, (quark, mass) in enumerate(quark_masses.items()):
|
| 103 |
+
particle_masses_evolution[j, 0] = particle_masses[j] # Initialize mass
|
| 104 |
+
|
| 105 |
+
for i in range(1, num_steps):
|
| 106 |
+
particle_speeds[j, i] = update_speed(
|
| 107 |
+
particle_speeds[j, i - 1],
|
| 108 |
+
particle_temperatures[j, i - 1],
|
| 109 |
+
particle_masses[j]
|
| 110 |
+
)
|
| 111 |
+
|
| 112 |
+
# Apply tunneling effect
|
| 113 |
+
if np.random.rand() < tunneling_probability:
|
| 114 |
+
particle_speeds[j, i] = particle_speeds[j, 0]
|
| 115 |
+
tunneling_steps[j, i] = True
|
| 116 |
+
|
| 117 |
+
particle_temperatures[j, i] = alpha * particle_speeds[j, i] ** 2 # Apply TSR equation
|
| 118 |
+
|
| 119 |
+
# Update mass based on energy conversion
|
| 120 |
+
energy_diff = relativistic_energy(particle_speeds[j, i], particle_masses[j]) - relativistic_energy(particle_speeds[j, i - 1], particle_masses[j])
|
| 121 |
+
particle_masses_evolution[j, i] = particle_masses_evolution[j, i - 1] + energy_diff / c**2
|
| 122 |
+
|
| 123 |
+
# Apply expansion of the universe
|
| 124 |
+
particle_speeds[j, i] *= 1 - Hubble_constant_SI * t_planck
|
| 125 |
+
particle_temperatures[j, i] *= 1 - Hubble_constant_SI * t_planck
|
| 126 |
+
|
| 127 |
+
# Check for collisions and handle them
|
| 128 |
+
collision, idx1, idx2 = check_collision(particle_speeds[:, i], collision_distance)
|
| 129 |
+
if collision:
|
| 130 |
+
handle_collision(particle_speeds[:, i], particle_masses, idx1, idx2)
|
| 131 |
+
|
| 132 |
+
# Print calculated masses at the end of the simulation
|
| 133 |
+
print(f"Calculated masses at the end of the simulation (Tunneling Probability: {tunneling_probability}):")
|
| 134 |
+
for j, quark in enumerate(quark_masses.keys()):
|
| 135 |
+
print(f"{quark}: {particle_masses_evolution[j, -1] / GeV_to_J:.4e} GeV")
|
| 136 |
+
|
| 137 |
+
# Save data to JSON file
|
| 138 |
+
data_filename = os.path.join(data_dir, f"big_bang_simulation_data_{tunneling_probability:.2f}.json")
|
| 139 |
+
data = {
|
| 140 |
+
"tunneling_probability": tunneling_probability,
|
| 141 |
+
"particle_masses_evolution": particle_masses_evolution.tolist(),
|
| 142 |
+
"particle_speeds": particle_speeds.tolist(),
|
| 143 |
+
"particle_temperatures": particle_temperatures.tolist(),
|
| 144 |
+
"tunneling_steps": tunneling_steps.tolist()
|
| 145 |
+
}
|
| 146 |
+
with open(data_filename, "w") as f:
|
| 147 |
+
json.dump(data, f)
|
sim2.py
ADDED
|
@@ -0,0 +1,152 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import numpy as np
|
| 2 |
+
import pandas as pd
|
| 3 |
+
import json
|
| 4 |
+
import os
|
| 5 |
+
|
| 6 |
+
# Constants
|
| 7 |
+
c = 299792458 # Speed of light in m/s
|
| 8 |
+
E_mc2 = c**2 # Mass-energy equivalence in J/kg
|
| 9 |
+
TSR = E_mc2 / (1.38e-23) # Temperature to Speed Ratio in K/m/s
|
| 10 |
+
alpha = 1.0 # Proportional constant for TSR
|
| 11 |
+
Q = 2 ** (1 / 12) # Fractal structure parameter
|
| 12 |
+
dark_energy_density = 5.96e-27 # Density of dark energy in kg/m^3
|
| 13 |
+
dark_matter_density = 2.25e-27 # Density of dark matter in kg/m^3
|
| 14 |
+
collision_distance = 1e-10 # Distance for collision detection
|
| 15 |
+
Hubble_constant = 70.0 # km/s/Mpc (approximation)
|
| 16 |
+
Hubble_constant_SI = (
|
| 17 |
+
Hubble_constant * 1000 / 3.086e22
|
| 18 |
+
) # Hubble constant in SI units (s^-1)
|
| 19 |
+
|
| 20 |
+
# Initial conditions
|
| 21 |
+
temperature_initial = 1.42e32 # Planck temperature in K
|
| 22 |
+
particle_density_initial = 5.16e96 # Planck density in kg/m^3
|
| 23 |
+
particle_speed_initial = c # Initially at the speed of light
|
| 24 |
+
|
| 25 |
+
# Simulation time
|
| 26 |
+
t_planck = 5.39e-44 # Planck time in s
|
| 27 |
+
t_simulation = t_planck * 1e5 # Shorter timescale for simulation
|
| 28 |
+
|
| 29 |
+
# Quark masses (in GeV) - used for initial mass values and comparison
|
| 30 |
+
quark_masses = {
|
| 31 |
+
"up": 2.3e-3,
|
| 32 |
+
"down": 4.8e-3,
|
| 33 |
+
"charm": 1.28,
|
| 34 |
+
"strange": 0.095,
|
| 35 |
+
"top": 173.0,
|
| 36 |
+
"bottom": 4.18,
|
| 37 |
+
"electron": 5.11e-4,
|
| 38 |
+
"muon": 1.05e-1,
|
| 39 |
+
"tau": 1.78,
|
| 40 |
+
"photon": 0,
|
| 41 |
+
}
|
| 42 |
+
|
| 43 |
+
# Conversion factor from GeV to J
|
| 44 |
+
GeV_to_J = 1.60217662e-10
|
| 45 |
+
|
| 46 |
+
# Simulation setup
|
| 47 |
+
num_steps = int(t_simulation / t_planck)
|
| 48 |
+
|
| 49 |
+
# Tunneling probabilities to investigate
|
| 50 |
+
tunneling_probabilities = np.arange(0.01, 2.5, 0.1) # Adjust range as needed
|
| 51 |
+
|
| 52 |
+
# Create a directory to store the data
|
| 53 |
+
data_dir = "big_bang_simulation_data"
|
| 54 |
+
os.makedirs(data_dir, exist_ok=True)
|
| 55 |
+
|
| 56 |
+
# Functions to incorporate relativistic effects and collisions
|
| 57 |
+
def relativistic_energy(particle_speed, particle_mass):
|
| 58 |
+
if particle_speed >= c:
|
| 59 |
+
return np.inf
|
| 60 |
+
return particle_mass * c**2 / np.sqrt(max(1e-10, 1 - (particle_speed / c) ** 2))
|
| 61 |
+
|
| 62 |
+
def relativistic_momentum(particle_speed, particle_mass):
|
| 63 |
+
if particle_speed >= c:
|
| 64 |
+
return np.inf
|
| 65 |
+
return (
|
| 66 |
+
particle_mass
|
| 67 |
+
* particle_speed
|
| 68 |
+
/ np.sqrt(max(1e-10, 1 - (particle_speed / c) ** 2))
|
| 69 |
+
)
|
| 70 |
+
|
| 71 |
+
def update_speed(current_speed, current_temperature, particle_mass):
|
| 72 |
+
rel_momentum = relativistic_momentum(current_speed, particle_mass)
|
| 73 |
+
return c * np.sqrt(
|
| 74 |
+
max(1e-10, 1 - (rel_momentum / (rel_momentum + dark_energy_density)) ** 2)
|
| 75 |
+
)
|
| 76 |
+
|
| 77 |
+
def check_collision(particle_speeds, collision_distance):
|
| 78 |
+
# Assuming 1D for simplicity. Expand for 3D if needed.
|
| 79 |
+
for j in range(len(particle_speeds)):
|
| 80 |
+
for k in range(j + 1, len(particle_speeds)):
|
| 81 |
+
if np.abs(particle_speeds[j] - particle_speeds[k]) < collision_distance:
|
| 82 |
+
return True, j, k
|
| 83 |
+
return False, -1, -1
|
| 84 |
+
|
| 85 |
+
def handle_collision(particle_speeds, idx1, idx2):
|
| 86 |
+
# Exchange momentum for a simplified collision response
|
| 87 |
+
p1 = relativistic_momentum(particle_speeds[idx1], particle_masses[idx1])
|
| 88 |
+
p2 = relativistic_momentum(particle_speeds[idx2], particle_masses[idx2])
|
| 89 |
+
|
| 90 |
+
# Simplified exchange
|
| 91 |
+
particle_speeds[idx1], particle_speeds[idx2] = p2 / particle_masses
|
| 92 |
+
[idx1], p1 / particle_masses[idx2]
|
| 93 |
+
|
| 94 |
+
# Simulate the Big Bang with Dark Energy, Dark Matter, Tunneling, and Relativistic Effects
|
| 95 |
+
for tunneling_probability in tunneling_probabilities:
|
| 96 |
+
print(f"Simulating for tunneling probability: {tunneling_probability}")
|
| 97 |
+
|
| 98 |
+
# Initialize arrays for simulation
|
| 99 |
+
particle_speeds = np.zeros((len(quark_masses), num_steps)) # 2D array for speeds
|
| 100 |
+
particle_temperatures = np.zeros((len(quark_masses), num_steps)) # 2D array for temperatures
|
| 101 |
+
particle_masses_evolution = np.zeros((len(quark_masses), num_steps)) # 2D array for mass evolution
|
| 102 |
+
tunneling_steps = np.zeros((len(quark_masses), num_steps), dtype=bool) # 2D array for tunneling steps
|
| 103 |
+
|
| 104 |
+
# Create an array of masses for each quark
|
| 105 |
+
particle_masses = np.array([mass * GeV_to_J for mass in quark_masses.values()])
|
| 106 |
+
|
| 107 |
+
for j, (quark, mass) in enumerate(quark_masses.items()):
|
| 108 |
+
# Initialize particle speeds and temperatures
|
| 109 |
+
particle_speeds[j, 0] = particle_speed_initial
|
| 110 |
+
particle_temperatures[j, 0] = temperature_initial
|
| 111 |
+
particle_masses_evolution[j, 0] = mass * GeV_to_J # Convert to Joules
|
| 112 |
+
|
| 113 |
+
# Time evolution loop
|
| 114 |
+
for step in range(1, num_steps):
|
| 115 |
+
for j in range(len(quark_masses)):
|
| 116 |
+
# Update temperature based on some model (placeholder)
|
| 117 |
+
particle_temperatures[j, step] = particle_temperatures[j, step - 1] * 0.99 # Cooling down
|
| 118 |
+
|
| 119 |
+
# Update speed based on temperature and mass
|
| 120 |
+
particle_speeds[j, step] = update_speed(
|
| 121 |
+
particle_speeds[j, step - 1],
|
| 122 |
+
particle_temperatures[j, step],
|
| 123 |
+
particle_masses[j]
|
| 124 |
+
)
|
| 125 |
+
|
| 126 |
+
# Check for collisions
|
| 127 |
+
collision_detected, idx1, idx2 = check_collision(particle_speeds[:, step], collision_distance)
|
| 128 |
+
if collision_detected:
|
| 129 |
+
handle_collision(particle_speeds[:, step], idx1, idx2)
|
| 130 |
+
|
| 131 |
+
# Tunneling effect (placeholder for actual physics)
|
| 132 |
+
if np.random.rand() < tunneling_probability:
|
| 133 |
+
tunneling_steps[j, step] = True
|
| 134 |
+
# Modify mass or speed based on tunneling (placeholder)
|
| 135 |
+
particle_masses[j] *= 1.1 # Increase mass as an example
|
| 136 |
+
|
| 137 |
+
# Store mass evolution
|
| 138 |
+
particle_masses_evolution[:, step] = particle_masses
|
| 139 |
+
|
| 140 |
+
# Save the simulation data for this tunneling probability
|
| 141 |
+
simulation_data = {
|
| 142 |
+
"particle_speeds": particle_speeds.tolist(), # Convert to list for JSON serialization
|
| 143 |
+
"particle_temperatures": particle_temperatures.tolist(), # Convert to list for JSON serialization
|
| 144 |
+
"particle_masses_evolution": particle_masses_evolution.tolist(), # Convert to list for JSON serialization
|
| 145 |
+
"tunneling_steps": tunneling_steps.tolist(), # Convert to list for JSON serialization
|
| 146 |
+
}
|
| 147 |
+
|
| 148 |
+
with open(os.path.join(data_dir, f"simulation_tunneling_{tunneling_probability:.2f}.json"), "w") as f:
|
| 149 |
+
json.dump(simulation_data, f)
|
| 150 |
+
|
| 151 |
+
print("Simulation completed and data saved.")
|
| 152 |
+
|
sim3.py
ADDED
|
@@ -0,0 +1,132 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import numpy as np
|
| 2 |
+
import json
|
| 3 |
+
import os
|
| 4 |
+
|
| 5 |
+
# Constants
|
| 6 |
+
c = 299792458 # Speed of light in m/s
|
| 7 |
+
E_mc2 = c**2 # Mass-energy equivalence in J/kg
|
| 8 |
+
dark_energy_density = 5.96e-27 # Density of dark energy in kg/m^3
|
| 9 |
+
collision_distance = 1e-10 # Distance for collision detection
|
| 10 |
+
|
| 11 |
+
# Initial conditions
|
| 12 |
+
temperature_initial = 1.42e32 # Planck temperature in K
|
| 13 |
+
particle_speed_initial = c # Initially at the speed of light
|
| 14 |
+
|
| 15 |
+
# Simulation time
|
| 16 |
+
t_planck = 5.39e-44 # Planck time in s
|
| 17 |
+
t_simulation = t_planck * 1e5 # Shorter timescale for simulation
|
| 18 |
+
|
| 19 |
+
# Quark masses (in GeV)
|
| 20 |
+
quark_masses = {
|
| 21 |
+
"up": 2.3e-3,
|
| 22 |
+
"down": 4.8e-3,
|
| 23 |
+
"charm": 1.28,
|
| 24 |
+
"strange": 0.095,
|
| 25 |
+
"top": 173.0,
|
| 26 |
+
"bottom": 4.18,
|
| 27 |
+
"electron": 5.11e-4,
|
| 28 |
+
"muon": 1.05e-1,
|
| 29 |
+
"tau": 1.78,
|
| 30 |
+
"photon": 0,
|
| 31 |
+
}
|
| 32 |
+
|
| 33 |
+
# Conversion factor from GeV to J
|
| 34 |
+
GeV_to_J = 1.60217662e-10
|
| 35 |
+
|
| 36 |
+
# Simulation setup
|
| 37 |
+
num_steps = int(t_simulation / t_planck)
|
| 38 |
+
|
| 39 |
+
# Create a directory to store the data
|
| 40 |
+
data_dir = "big_bang_simulation_data"
|
| 41 |
+
os.makedirs(data_dir, exist_ok=True)
|
| 42 |
+
|
| 43 |
+
# Functions to incorporate relativistic effects and collisions
|
| 44 |
+
def relativistic_momentum(particle_speed, particle_mass):
|
| 45 |
+
if particle_speed >= c:
|
| 46 |
+
return np.inf
|
| 47 |
+
return (
|
| 48 |
+
particle_mass
|
| 49 |
+
* particle_speed
|
| 50 |
+
/ np.sqrt(max(1e-10, 1 - (particle_speed / c) ** 2))
|
| 51 |
+
)
|
| 52 |
+
|
| 53 |
+
def update_speed(current_speed, current_temperature, particle_mass):
|
| 54 |
+
# Placeholder for speed update logic
|
| 55 |
+
return current_speed # This should be replaced with actual logic
|
| 56 |
+
|
| 57 |
+
def check_collision(particle_speeds, collision_distance):
|
| 58 |
+
for j in range(len(particle_speeds)):
|
| 59 |
+
for k in range(j + 1, len(particle_speeds)):
|
| 60 |
+
if np.abs(particle_speeds[j] - particle_speeds[k]) < collision_distance:
|
| 61 |
+
return True, j, k
|
| 62 |
+
return False, -1, -1
|
| 63 |
+
|
| 64 |
+
def handle_collision(particle_speeds, idx1, idx2):
|
| 65 |
+
# Exchange momentum for a simplified collision response
|
| 66 |
+
p1 = relativistic_momentum(particle_speeds[idx1], particle_masses[idx1])
|
| 67 |
+
p2 = relativistic_momentum(particle_speeds[idx2], particle_masses[idx2])
|
| 68 |
+
|
| 69 |
+
# Simplified exchange of speeds based on momentum
|
| 70 |
+
particle_speeds[idx1] = p2 / particle_masses[idx1] # Update speed of particle 1
|
| 71 |
+
particle_speeds[idx2] = p1 / particle_masses[idx2] # Update speed of particle 2
|
| 72 |
+
|
| 73 |
+
# Simulate the Big Bang with Dark Energy, Dark Matter, Tunneling, and Relativistic Effects
|
| 74 |
+
for tunneling_probability in np.arange(0.01, 2.5, 0.1):
|
| 75 |
+
print(f"Simulating for tunneling probability: {tunneling_probability}")
|
| 76 |
+
|
| 77 |
+
# Initialize arrays for simulation
|
| 78 |
+
particle_speeds = np.zeros((len(quark_masses), num_steps)) # 2D array for speeds
|
| 79 |
+
particle_temperatures = np.zeros((len(quark_masses), num_steps)) # 2D array for temperatures
|
| 80 |
+
np.zeros((len(quark_masses), num_steps)) # 2D array for temperatures
|
| 81 |
+
particle_masses_evolution = np.zeros((len(quark_masses), num_steps)) # 2D array for mass evolution
|
| 82 |
+
tunneling_steps = np.zeros((len(quark_masses), num_steps), dtype=bool) # 2D array for tunneling steps
|
| 83 |
+
|
| 84 |
+
# Create an array of masses for each quark
|
| 85 |
+
particle_masses = np.array([mass * GeV_to_J for mass in quark_masses.values()])
|
| 86 |
+
|
| 87 |
+
for j, (quark, mass) in enumerate(quark_masses.items()):
|
| 88 |
+
# Initialize particle speeds and temperatures
|
| 89 |
+
particle_speeds[j, 0] = particle_speed_initial
|
| 90 |
+
particle_temperatures[j, 0] = temperature_initial
|
| 91 |
+
particle_masses_evolution[j, 0] = mass * GeV_to_J # Convert to Joules
|
| 92 |
+
|
| 93 |
+
# Time evolution loop
|
| 94 |
+
for step in range(1, num_steps):
|
| 95 |
+
for j in range(len(quark_masses)):
|
| 96 |
+
# Update temperature based on some model (placeholder)
|
| 97 |
+
particle_temperatures[j, step] = particle_temperatures[j, step - 1] * 0.99 # Cooling down
|
| 98 |
+
|
| 99 |
+
# Update speed based on temperature and mass
|
| 100 |
+
particle_speeds[j, step] = update_speed(
|
| 101 |
+
particle_speeds[j, step - 1],
|
| 102 |
+
particle_temperatures[j, step],
|
| 103 |
+
particle_masses[j]
|
| 104 |
+
)
|
| 105 |
+
|
| 106 |
+
# Check for collisions
|
| 107 |
+
collision_detected, idx1, idx2 = check_collision(particle_speeds[:, step], collision_distance)
|
| 108 |
+
if collision_detected:
|
| 109 |
+
handle_collision(particle_speeds[:, step], idx1, idx2)
|
| 110 |
+
|
| 111 |
+
# Tunneling effect (placeholder for actual physics)
|
| 112 |
+
if np.random.rand() < tunneling_probability:
|
| 113 |
+
tunneling_steps[j, step] = True
|
| 114 |
+
# Modify mass or speed based on tunneling (placeholder)
|
| 115 |
+
particle_masses[j] *= 1.1 # Increase mass as an example
|
| 116 |
+
|
| 117 |
+
# Store mass evolution
|
| 118 |
+
particle_masses_evolution[:, step] = particle_masses
|
| 119 |
+
|
| 120 |
+
# Save the simulation data for this tunneling probability
|
| 121 |
+
simulation_data = {
|
| 122 |
+
"particle_speeds": particle_speeds.tolist(), # Convert to list for JSON serialization
|
| 123 |
+
"particle_temperatures": particle_temperatures.tolist(), # Convert to list for JSON serialization
|
| 124 |
+
"particle_masses_evolution": particle_masses_evolution.tolist(), # Convert to list for JSON serialization
|
| 125 |
+
"tunneling_steps": tunneling_steps.tolist(), # Convert to list for JSON serialization
|
| 126 |
+
}
|
| 127 |
+
|
| 128 |
+
with open(os.path.join(data_dir, f"simulation_tunneling_{tunneling_probability:.2f}.json"), "w") as f:
|
| 129 |
+
json.dump(simulation_data, f)
|
| 130 |
+
|
| 131 |
+
print("Simulation completed and data saved.")
|
| 132 |
+
|
sim8.py
ADDED
|
@@ -0,0 +1,181 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import numpy as np
|
| 2 |
+
import numba
|
| 3 |
+
from numba import cuda
|
| 4 |
+
import dask
|
| 5 |
+
from dask import delayed
|
| 6 |
+
from dask.diagnostics import ProgressBar
|
| 7 |
+
import time
|
| 8 |
+
from scipy.stats import norm
|
| 9 |
+
|
| 10 |
+
# Constants
|
| 11 |
+
c = 299792458 # Speed of light in m/s
|
| 12 |
+
E_mc2 = c**2 # Mass-energy equivalence in J/kg
|
| 13 |
+
TSR = E_mc2 / (1.38e-23) # Temperature to Speed Ratio in K/m/s
|
| 14 |
+
alpha = 1.0 # Proportional constant for TSR
|
| 15 |
+
Q = 2 ** (1 / 12) # Fractal structure parameter
|
| 16 |
+
dark_energy_density = 5.96e-27 # Density of dark energy in kg/m^3
|
| 17 |
+
dark_matter_density = 2.25e-27 # Density of dark matter in kg/m^3
|
| 18 |
+
collision_distance = 1e-10 # Distance for collision detection
|
| 19 |
+
Hubble_constant = 70.0 # km/s/Mpc (approximation)
|
| 20 |
+
Hubble_constant_SI = (
|
| 21 |
+
Hubble_constant * 1000 / 3.086e22
|
| 22 |
+
) # Hubble constant in SI units (s^-1)
|
| 23 |
+
|
| 24 |
+
# Initial conditions
|
| 25 |
+
temperature_initial = 1.42e32 # Planck temperature in K
|
| 26 |
+
particle_density_initial = 5.16e96 # Planck density in kg/m^3
|
| 27 |
+
particle_speed_initial = c # Initially at the speed of light
|
| 28 |
+
|
| 29 |
+
# Simulation time
|
| 30 |
+
t_planck = 5.39e-44 # Planck time in s
|
| 31 |
+
t_simulation = t_planck * 1e3 # Shorter timescale for simulation
|
| 32 |
+
|
| 33 |
+
# Quark masses (in GeV) - used for initial mass values and comparison
|
| 34 |
+
quark_masses = {
|
| 35 |
+
"up": 2.3e-3,
|
| 36 |
+
"down": 4.8e-3,
|
| 37 |
+
"charm": 1.28,
|
| 38 |
+
"strange": 0.095,
|
| 39 |
+
"top": 173.0,
|
| 40 |
+
"bottom": 4.18,
|
| 41 |
+
}
|
| 42 |
+
|
| 43 |
+
# **ASK FOR NUMBER OF PARTICLES**
|
| 44 |
+
while True:
|
| 45 |
+
try:
|
| 46 |
+
num_particles = int(input("Enter the number of particles (integer): "))
|
| 47 |
+
if num_particles <= 0:
|
| 48 |
+
print("Please enter a positive integer.")
|
| 49 |
+
else:
|
| 50 |
+
break
|
| 51 |
+
except ValueError:
|
| 52 |
+
print("Invalid input. Please enter an integer.")
|
| 53 |
+
|
| 54 |
+
# **ASK FOR TUNNELING PROBABILITY**
|
| 55 |
+
while True:
|
| 56 |
+
try:
|
| 57 |
+
tunneling_probability = float(input("Enter the tunneling probability (float, 0-1): "))
|
| 58 |
+
if 0 <= tunneling_probability <= 1:
|
| 59 |
+
break
|
| 60 |
+
else:
|
| 61 |
+
print("Please enter a value between 0 and 1.")
|
| 62 |
+
except ValueError:
|
| 63 |
+
print("Invalid input. Please enter a float.")
|
| 64 |
+
|
| 65 |
+
# Generate additional particles based on user input
|
| 66 |
+
additional_particles = {
|
| 67 |
+
f"new_quark_{i}": np.random.uniform(1e-3, 1e-1) for i in range(num_particles - len(quark_masses))
|
| 68 |
+
}
|
| 69 |
+
|
| 70 |
+
all_particles = {**quark_masses, **additional_particles}
|
| 71 |
+
|
| 72 |
+
# Conversion factor from GeV to J
|
| 73 |
+
GeV_to_J = 1.60217662e-10
|
| 74 |
+
|
| 75 |
+
# Simulation setup
|
| 76 |
+
num_steps = int(t_simulation / t_planck)
|
| 77 |
+
|
| 78 |
+
# CUDA kernel for simulation step
|
| 79 |
+
@cuda.jit
|
| 80 |
+
def simulation_step(particle_speeds, particle_temperatures, particle_masses, step, tunneling_probability):
|
| 81 |
+
tx = cuda.threadIdx.x
|
| 82 |
+
bx = cuda.blockIdx.x
|
| 83 |
+
bw = cuda.blockDim.x
|
| 84 |
+
i = tx + bx * bw
|
| 85 |
+
|
| 86 |
+
if i < num_particles:
|
| 87 |
+
# Update speed
|
| 88 |
+
particle_speeds[i] = update_speed(
|
| 89 |
+
particle_speeds[i], particle_temperatures[i], particle_masses[i]
|
| 90 |
+
)
|
| 91 |
+
|
| 92 |
+
# Apply tunneling probability
|
| 93 |
+
if np.random.rand() < tunneling_probability:
|
| 94 |
+
particle_speeds[i] = particle_speed_initial
|
| 95 |
+
|
| 96 |
+
# Update temperature
|
| 97 |
+
particle_temperatures[i] = alpha * particle_speeds[i] ** 2
|
| 98 |
+
|
| 99 |
+
# Simple collision detection (for demonstration; enhance as needed)
|
| 100 |
+
for j in range(num_particles):
|
| 101 |
+
if i != j:
|
| 102 |
+
# Collision logic here (omitted for brevity)
|
| 103 |
+
pass # Placeholder for collision logic
|
| 104 |
+
|
| 105 |
+
# CPU function for updating speed (example; optimize as necessary)
|
| 106 |
+
def update_speed(current_speed, current_temperature, particle_mass):
|
| 107 |
+
rel_momentum = relativistic_momentum(current_speed, particle_mass)
|
| 108 |
+
return c * np.sqrt(
|
| 109 |
+
max(1e-10, 1 - (rel_momentum / (rel_momentum + dark_energy_density)) ** 2)
|
| 110 |
+
)
|
| 111 |
+
|
| 112 |
+
# CPU function for relativistic momentum (example; optimize as necessary)
|
| 113 |
+
def relativistic_momentum(particle_speed, particle_mass):
|
| 114 |
+
if particle_speed >= c:
|
| 115 |
+
return np.inf
|
| 116 |
+
return (
|
| 117 |
+
particle_mass
|
| 118 |
+
* particle_speed
|
| 119 |
+
/ np.sqrt(max(1e-10, 1 - (particle_speed / c) ** 2))
|
| 120 |
+
)
|
| 121 |
+
|
| 122 |
+
# Generate additional particles based on user input
|
| 123 |
+
additional_particles = {
|
| 124 |
+
f"new_quark_{i}": np.random.uniform(1e-3, 1e-1) for i in range(num_particles - len(quark_masses))
|
| 125 |
+
}
|
| 126 |
+
|
| 127 |
+
# Ensure that the number of particles is at least the number of quark masses
|
| 128 |
+
if num_particles < len(quark_masses):
|
| 129 |
+
print(f"Warning: Reducing the number of particles to {len(quark_masses)} to match quark masses.")
|
| 130 |
+
num_particles = len(quark_masses)
|
| 131 |
+
|
| 132 |
+
all_particles = {**quark_masses, **additional_particles}
|
| 133 |
+
|
| 134 |
+
# Initialize particle properties
|
| 135 |
+
initial_speeds = np.full(num_particles, particle_speed_initial, dtype=np.float64)
|
| 136 |
+
initial_temperatures = np.full(num_particles, temperature_initial, dtype=np.float64)
|
| 137 |
+
|
| 138 |
+
# Create an array of masses based on the number of particles
|
| 139 |
+
initial_masses = np.zeros(num_particles, dtype=np.float64)
|
| 140 |
+
|
| 141 |
+
# Fill initial_masses with quark masses and additional particles
|
| 142 |
+
for i, (key, mass) in enumerate(all_particles.items()):
|
| 143 |
+
if i < num_particles:
|
| 144 |
+
initial_masses[i] = mass
|
| 145 |
+
|
| 146 |
+
# Main simulation loop
|
| 147 |
+
def main_simulation(tunneling_probability):
|
| 148 |
+
# Memory allocation for simulation arrays
|
| 149 |
+
d_particle_speeds = cuda.device_array(num_particles, dtype=np.float64)
|
| 150 |
+
d_particle_temperatures = cuda.device_array(num_particles, dtype=np.float64)
|
| 151 |
+
d_particle_masses = cuda.device_array(num_particles, dtype=np.float64)
|
| 152 |
+
|
| 153 |
+
# Copy initial values to device
|
| 154 |
+
d_particle_speeds.copy_to_device(initial_speeds)
|
| 155 |
+
d_particle_temperatures.copy_to_device(initial_temperatures)
|
| 156 |
+
d_particle_masses.copy_to_device(initial_masses)
|
| 157 |
+
|
| 158 |
+
# Simulation loop
|
| 159 |
+
for step in range(num_steps):
|
| 160 |
+
simulation_step[1, num_particles](d_particle_speeds, d_particle_temperatures, d_particle_masses, step, tunneling_probability)
|
| 161 |
+
|
| 162 |
+
# Copy results back to host
|
| 163 |
+
h_particle_speeds = d_particle_speeds.copy_to_host()
|
| 164 |
+
h_particle_temperatures = d_particle_temperatures.copy_to_host()
|
| 165 |
+
h_particle_masses = d_particle_masses.copy_to_host()
|
| 166 |
+
|
| 167 |
+
return h_particle_speeds, h_particle_temperatures, h_particle_masses
|
| 168 |
+
|
| 169 |
+
if __name__ == "__main__":
|
| 170 |
+
start_time = time.time()
|
| 171 |
+
with ProgressBar():
|
| 172 |
+
task = delayed(main_simulation)(tunneling_probability)
|
| 173 |
+
result = task.compute()
|
| 174 |
+
end_time = time.time()
|
| 175 |
+
print(f"Simulation completed in {end_time - start_time} seconds")
|
| 176 |
+
|
| 177 |
+
# Process and visualize results as needed
|
| 178 |
+
particle_speeds, particle_temperatures, particle_masses = result
|
| 179 |
+
print("Final Particle Speeds:", particle_speeds)
|
| 180 |
+
print("Final Particle Temperatures:", particle_temperatures)
|
| 181 |
+
print("Final Particle Masses:", particle_masses)
|
sim9.py
ADDED
|
@@ -0,0 +1,181 @@
|
|
|
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|
|
|
|
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|
|
|
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|
|
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|
|
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|
|
|
|
|
|
|
|
|
|
|
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|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import numpy as np
|
| 2 |
+
import pandas as pd
|
| 3 |
+
import json
|
| 4 |
+
import os
|
| 5 |
+
|
| 6 |
+
# Constants
|
| 7 |
+
c = 299792458 # Speed of light in m/s
|
| 8 |
+
E_mc2 = c**2 # Mass-energy equivalence in J/kg
|
| 9 |
+
TSR = E_mc2 / (1.38e-23) # Temperature to Speed Ratio in K/m/s
|
| 10 |
+
alpha = 1.0 # Proportional constant for TSR
|
| 11 |
+
Q = 2 ** (1 / 12) # Fractal structure parameter
|
| 12 |
+
dark_energy_density = 5.96e-27 # Density of dark energy in kg/m^3
|
| 13 |
+
dark_matter_density = 2.25e-27 # Density of dark matter in kg/m^3
|
| 14 |
+
collision_distance = 1e-10 # Distance for collision detection
|
| 15 |
+
Hubble_constant = 70.0 # km/s/Mpc (approximation)
|
| 16 |
+
Hubble_constant_SI = (
|
| 17 |
+
Hubble_constant * 1000 / 3.086e22
|
| 18 |
+
) # Hubble constant in SI units (s^-1)
|
| 19 |
+
|
| 20 |
+
# Initial conditions
|
| 21 |
+
temperature_initial = 1.42e32 # Planck temperature in K
|
| 22 |
+
particle_density_initial = 5.16e96 # Planck density in kg/m^3
|
| 23 |
+
particle_speed_initial = c # Initially at the speed of light
|
| 24 |
+
|
| 25 |
+
# Simulation time
|
| 26 |
+
t_planck = 5.39e-44 # Planck time in s
|
| 27 |
+
t_simulation = t_planck * 1e5 # Shorter timescale for simulation
|
| 28 |
+
|
| 29 |
+
# Quark masses (in GeV) - used for initial mass values and comparison
|
| 30 |
+
quark_masses = {
|
| 31 |
+
"up": 2.3e-3,
|
| 32 |
+
"down": 4.8e-3,
|
| 33 |
+
"charm": 1.28,
|
| 34 |
+
"strange": 0.095,
|
| 35 |
+
"top": 173.0,
|
| 36 |
+
"bottom": 4.18,
|
| 37 |
+
"electron": 5.11e-4,
|
| 38 |
+
"muon": 1.05e-1,
|
| 39 |
+
"tau": 1.78,
|
| 40 |
+
"photon": 0,
|
| 41 |
+
}
|
| 42 |
+
|
| 43 |
+
# Conversion factor from GeV to J
|
| 44 |
+
GeV_to_J = 1.60217662e-10
|
| 45 |
+
|
| 46 |
+
# Simulation setup
|
| 47 |
+
num_steps = int(t_simulation / t_planck)
|
| 48 |
+
|
| 49 |
+
# Tunneling probabilities to investigate
|
| 50 |
+
tunneling_probabilities = np.arange(0.1, 1.1, 0.1) # Exclude 1.0
|
| 51 |
+
|
| 52 |
+
# Create a directory to store the data
|
| 53 |
+
data_dir = "big_bang_simulation_data"
|
| 54 |
+
os.makedirs(data_dir, exist_ok=True)
|
| 55 |
+
|
| 56 |
+
# Functions to incorporate relativistic effects
|
| 57 |
+
def relativistic_energy(particle_speed, particle_mass):
|
| 58 |
+
if particle_speed >= c:
|
| 59 |
+
return np.inf
|
| 60 |
+
return particle_mass * c**2 / np.sqrt(max(1e-10, 1 - (particle_speed / c) ** 2))
|
| 61 |
+
|
| 62 |
+
|
| 63 |
+
def relativistic_momentum(particle_speed, particle_mass):
|
| 64 |
+
if particle_speed >= c:
|
| 65 |
+
return np.inf
|
| 66 |
+
return (
|
| 67 |
+
particle_mass
|
| 68 |
+
* particle_speed
|
| 69 |
+
/ np.sqrt(max(1e-10, 1 - (particle_speed / c) ** 2))
|
| 70 |
+
)
|
| 71 |
+
|
| 72 |
+
|
| 73 |
+
def update_speed(current_speed, current_temperature, particle_mass):
|
| 74 |
+
rel_momentum = relativistic_momentum(current_speed, particle_mass)
|
| 75 |
+
return c * np.sqrt(
|
| 76 |
+
max(1e-10, 1 - (rel_momentum / (rel_momentum + dark_energy_density)) ** 2)
|
| 77 |
+
)
|
| 78 |
+
|
| 79 |
+
|
| 80 |
+
# Simulate the Big Bang with Dark Energy, Dark Matter, Tunneling, and Relativistic Effects
|
| 81 |
+
for tunneling_probability in tunneling_probabilities:
|
| 82 |
+
print(f"Simulating for tunneling probability: {tunneling_probability}")
|
| 83 |
+
|
| 84 |
+
# Initialize arrays for simulation
|
| 85 |
+
particle_speeds = np.zeros((len(quark_masses), num_steps)) # 2D array for speeds
|
| 86 |
+
particle_temperatures = np.zeros(
|
| 87 |
+
(len(quark_masses), num_steps)
|
| 88 |
+
) # 2D array for temperatures
|
| 89 |
+
particle_masses_evolution = np.zeros(
|
| 90 |
+
(len(quark_masses), num_steps)
|
| 91 |
+
) # 2D array for mass evolution
|
| 92 |
+
tunneling_steps = np.zeros(
|
| 93 |
+
(len(quark_masses), num_steps), dtype=bool
|
| 94 |
+
) # 2D array for tunneling steps
|
| 95 |
+
|
| 96 |
+
# Create an array of masses for each quark
|
| 97 |
+
particle_masses = np.array([mass * GeV_to_J for mass in quark_masses.values()])
|
| 98 |
+
|
| 99 |
+
for j, (quark, mass) in enumerate(quark_masses.items()):
|
| 100 |
+
particle_masses_evolution[j, 0] = particle_masses[j] # Initialize mass
|
| 101 |
+
|
| 102 |
+
for i in range(1, num_steps):
|
| 103 |
+
particle_speeds[j, i] = update_speed(
|
| 104 |
+
particle_speeds[j, i - 1],
|
| 105 |
+
particle_temperatures[j, i - 1],
|
| 106 |
+
particle_masses[j],
|
| 107 |
+
)
|
| 108 |
+
|
| 109 |
+
value = (
|
| 110 |
+
1
|
| 111 |
+
- (particle_speeds[j, i] / (TSR * temperature_initial))
|
| 112 |
+
+ dark_matter_density
|
| 113 |
+
)
|
| 114 |
+
|
| 115 |
+
if np.random.rand() < tunneling_probability:
|
| 116 |
+
particle_speeds[j, i] = particle_speeds[j, 0] # Tunneling effect
|
| 117 |
+
tunneling_steps[j, i] = True # Mark tunneling step
|
| 118 |
+
|
| 119 |
+
if value < 0:
|
| 120 |
+
value = 0
|
| 121 |
+
|
| 122 |
+
particle_temperatures[j, i] = (
|
| 123 |
+
alpha * particle_speeds[j, i] ** 2
|
| 124 |
+
) # Apply TSR equation
|
| 125 |
+
|
| 126 |
+
# Update mass based on energy conversion
|
| 127 |
+
speed_squared_diff = (
|
| 128 |
+
particle_speeds[j, i] ** 2 - particle_speeds[j, i - 1] ** 2
|
| 129 |
+
)
|
| 130 |
+
|
| 131 |
+
# Avoid division by zero (if speed doesn't change, mass doesn't change)
|
| 132 |
+
if speed_squared_diff == 0:
|
| 133 |
+
particle_masses_evolution[j, i] = particle_masses_evolution[j, i - 1]
|
| 134 |
+
else:
|
| 135 |
+
# Calculate the change in relativistic energy
|
| 136 |
+
energy_diff = relativistic_energy(
|
| 137 |
+
particle_speeds[j, i], particle_masses[j]
|
| 138 |
+
) - relativistic_energy(particle_speeds[j, i - 1], particle_masses[j])
|
| 139 |
+
|
| 140 |
+
# Avoid NaN by checking if energy_diff is practically zero
|
| 141 |
+
if abs(energy_diff) < 1e-15: # Adjust the tolerance as needed
|
| 142 |
+
particle_masses_evolution[j, i] = particle_masses_evolution[
|
| 143 |
+
j, i - 1
|
| 144 |
+
]
|
| 145 |
+
else:
|
| 146 |
+
# Update mass based on energy difference
|
| 147 |
+
new_mass = (
|
| 148 |
+
particle_masses_evolution[j, i - 1] + energy_diff / c**2
|
| 149 |
+
)
|
| 150 |
+
if np.isfinite(new_mass): # Check if the new mass is finite
|
| 151 |
+
particle_masses_evolution[j, i] = new_mass
|
| 152 |
+
else:
|
| 153 |
+
particle_masses_evolution[j, i] = particle_masses_evolution[
|
| 154 |
+
j, i - 1
|
| 155 |
+
]
|
| 156 |
+
|
| 157 |
+
# Apply expansion of the universe (redshift)
|
| 158 |
+
particle_speeds[j, i] *= 1 - Hubble_constant_SI * t_planck
|
| 159 |
+
|
| 160 |
+
# Apply expansion of the universe (cooling)
|
| 161 |
+
particle_temperatures[j, i] *= 1 - Hubble_constant_SI * t_planck
|
| 162 |
+
|
| 163 |
+
# Print calculated masses at the end of the simulation
|
| 164 |
+
print(
|
| 165 |
+
f"Calculated masses at the end of the simulation (Tunneling Probability: {tunneling_probability}):"
|
| 166 |
+
)
|
| 167 |
+
for j, quark in enumerate(quark_masses.keys()):
|
| 168 |
+
print(
|
| 169 |
+
f"{quark}: {particle_masses_evolution[j, -1] / GeV_to_J:.4e} GeV"
|
| 170 |
+
)
|
| 171 |
+
|
| 172 |
+
# Save data to JSON file
|
| 173 |
+
data_filename = os.path.join(
|
| 174 |
+
data_dir, f"big_bang_simulation_data_{tunneling_probability:.1f}.json"
|
| 175 |
+
)
|
| 176 |
+
data = {
|
| 177 |
+
"tunneling_probability": tunneling_probability,
|
| 178 |
+
"particle_masses_evolution": particle_masses_evolution.tolist(),
|
| 179 |
+
}
|
| 180 |
+
with open(data_filename, "w") as f:
|
| 181 |
+
json.dump(data, f)
|
simA.py
ADDED
|
@@ -0,0 +1,146 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import streamlit as st
|
| 2 |
+
|
| 3 |
+
x = st.slider('Select a value')
|
| 4 |
+
st.write(x, 'squared is', x * x)
|
| 5 |
+
|
| 6 |
+
import numpy as np
|
| 7 |
+
import pandas as pd
|
| 8 |
+
import json
|
| 9 |
+
import os
|
| 10 |
+
|
| 11 |
+
# Constants
|
| 12 |
+
c = 299792458 # Speed of light in m/s
|
| 13 |
+
E_mc2 = c**2 # Mass-energy equivalence in J/kg
|
| 14 |
+
TSR = E_mc2 / (1.38e-23) # Temperature to Speed Ratio in K/m/s
|
| 15 |
+
alpha = 1.0 # Proportional constant for TSR
|
| 16 |
+
Q = 2 ** (1 / 12) # Fractal structure parameter
|
| 17 |
+
dark_energy_density = 5.96e-27 # Density of dark energy in kg/m^3
|
| 18 |
+
dark_matter_density = 2.25e-27 # Density of dark matter in kg/m^3
|
| 19 |
+
collision_distance = 1e-10 # Distance for collision detection
|
| 20 |
+
Hubble_constant = 70.0 # km/s/Mpc (approximation)
|
| 21 |
+
Hubble_constant_SI = Hubble_constant * 1000 / 3.086e22 # Convert to SI units (s^-1)
|
| 22 |
+
|
| 23 |
+
# Initial conditions
|
| 24 |
+
temperature_initial = 1.0 # Planck temperature in K
|
| 25 |
+
particle_density_initial = 5.16e96 # Planck density in kg/m^3
|
| 26 |
+
particle_speed_initial = TSR * temperature_initial # Initial speed based on TSR
|
| 27 |
+
|
| 28 |
+
# Simulation time
|
| 29 |
+
t_planck = 5.39e-44 # Planck time in s
|
| 30 |
+
t_simulation = t_planck * 1e5 # Shorter timescale for simulation
|
| 31 |
+
|
| 32 |
+
# Quark masses (in GeV) - used for initial mass values and comparison
|
| 33 |
+
quark_masses = {
|
| 34 |
+
"up": 2.3e-3,
|
| 35 |
+
"down": 4.8e-3,
|
| 36 |
+
"charm": 1.28,
|
| 37 |
+
"strange": 0.095,
|
| 38 |
+
"top": 173.0,
|
| 39 |
+
"bottom": 4.18,
|
| 40 |
+
"electron": 5.11e-4,
|
| 41 |
+
"muon": 1.05e-1,
|
| 42 |
+
"tau": 1.78,
|
| 43 |
+
"photon": 0,
|
| 44 |
+
}
|
| 45 |
+
|
| 46 |
+
# Conversion factor from GeV to J
|
| 47 |
+
GeV_to_J = 1.60217662e-10
|
| 48 |
+
|
| 49 |
+
# Simulation setup
|
| 50 |
+
num_steps = int(t_simulation / t_planck)
|
| 51 |
+
|
| 52 |
+
# Tunneling probabilities to investigate
|
| 53 |
+
tunneling_probabilities = np.arange(0.000001, 150, 10)
|
| 54 |
+
# Create a directory to store the data
|
| 55 |
+
data_dir = "big_bang_simulation_data"
|
| 56 |
+
os.makedirs(data_dir, exist_ok=True)
|
| 57 |
+
|
| 58 |
+
# Functions to incorporate relativistic effects and collisions
|
| 59 |
+
def relativistic_energy(particle_speed, particle_mass):
|
| 60 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 61 |
+
return particle_mass * c**2 / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 62 |
+
|
| 63 |
+
def relativistic_momentum(particle_speed, particle_mass):
|
| 64 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 65 |
+
return particle_mass * particle_speed / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 66 |
+
|
| 67 |
+
def update_speed(current_speed, current_temperature, particle_mass):
|
| 68 |
+
"""Update the speed of a particle based on temperature and mass."""
|
| 69 |
+
return TSR * current_temperature # Update speed using TSR
|
| 70 |
+
|
| 71 |
+
def check_collision(particle_speeds, collision_distance):
|
| 72 |
+
epsilon = 1e-15 # A small value to avoid invalid subtraction
|
| 73 |
+
for j in range(len(particle_speeds)):
|
| 74 |
+
for k in range(j+1, len(particle_speeds)):
|
| 75 |
+
if np.abs(particle_speeds[j] - particle_speeds[k]) < collision_distance + epsilon:
|
| 76 |
+
return True, j, k
|
| 77 |
+
return False, -1, -1
|
| 78 |
+
|
| 79 |
+
def handle_collision(particle_speeds, particle_masses, idx1, idx2):
|
| 80 |
+
"""Handle a collision between two particles."""
|
| 81 |
+
p1 = relativistic_momentum(particle_speeds[idx1], particle_masses[idx1])
|
| 82 |
+
p2 = relativistic_momentum(particle_speeds[idx2], particle_masses[idx2])
|
| 83 |
+
|
| 84 |
+
# Calculate velocities after collision using conservation of momentum
|
| 85 |
+
total_momentum = p1 + p2
|
| 86 |
+
total_mass = particle_masses[idx1] + particle_masses[idx2]
|
| 87 |
+
v1_new = (total_momentum / total_mass) * (particle_masses[idx1] / total_mass)
|
| 88 |
+
v2_new = (total_momentum / total_mass) * (particle_masses[idx2] / total_mass)
|
| 89 |
+
|
| 90 |
+
particle_speeds[idx1], particle_speeds[idx2] = v1_new, v2_new
|
| 91 |
+
|
| 92 |
+
# Simulate the Big Bang with Dark Energy, Dark Matter, Tunneling, and Relativistic Effects
|
| 93 |
+
for tunneling_probability in tunneling_probabilities:
|
| 94 |
+
print(f"Simulating for tunneling probability: {tunneling_probability}")
|
| 95 |
+
|
| 96 |
+
# Initialize arrays for simulation
|
| 97 |
+
particle_speeds = np.zeros((len(quark_masses), num_steps)) # 2D array for speeds
|
| 98 |
+
particle_temperatures = np.zeros((len(quark_masses), num_steps)) # 2D array for temperatures
|
| 99 |
+
particle_masses_evolution = np.zeros((len(quark_masses), num_steps)) # 2D array for mass evolution
|
| 100 |
+
tunneling_steps = np.zeros((len(quark_masses), num_steps), dtype=bool) # 2D array for tunneling steps
|
| 101 |
+
|
| 102 |
+
# Create an array of masses for each quark
|
| 103 |
+
particle_masses = np.array([mass * GeV_to_J for mass in quark_masses.values()])
|
| 104 |
+
|
| 105 |
+
for j, (quark, mass) in enumerate(quark_masses.items()):
|
| 106 |
+
particle_masses_evolution[j, 0] = particle_masses[j] # Initialize mass
|
| 107 |
+
particle_speeds[j, 0] = particle_speed_initial # Initialize speed
|
| 108 |
+
particle_temperatures[j, 0] = temperature_initial # Initialize temperature
|
| 109 |
+
|
| 110 |
+
for i in range(1, num_steps):
|
| 111 |
+
# Update temperature based on expansion of the universe
|
| 112 |
+
particle_temperatures[j, i] = particle_temperatures[j, i-1] * (1 - Hubble_constant_SI * t_planck)
|
| 113 |
+
|
| 114 |
+
# Update speed using TSR
|
| 115 |
+
particle_speeds[j, i] = update_speed(particle_speeds[j, i-1], particle_temperatures[j, i], particle_masses[j])
|
| 116 |
+
|
| 117 |
+
# Apply tunneling effect
|
| 118 |
+
if np.random.rand() < tunneling_probability:
|
| 119 |
+
particle_speeds[j, i] = particle_speeds[j, 0]
|
| 120 |
+
tunneling_steps[j, i] = True
|
| 121 |
+
|
| 122 |
+
# Update mass based on energy conversion
|
| 123 |
+
energy_diff = relativistic_energy(particle_speeds[j, i], particle_masses[j]) - relativistic_energy(particle_speeds[j, i - 1], particle_masses[j])
|
| 124 |
+
particle_masses_evolution[j, i] = particle_masses_evolution[j, i - 1] + energy_diff / c**2
|
| 125 |
+
|
| 126 |
+
# Check for collisions and handle them
|
| 127 |
+
collision, idx1, idx2 = check_collision(particle_speeds[:, i], collision_distance)
|
| 128 |
+
if collision:
|
| 129 |
+
handle_collision(particle_speeds[:, i], particle_masses, idx1, idx2)
|
| 130 |
+
|
| 131 |
+
# Print calculated masses at the end of the simulation
|
| 132 |
+
print(f"Calculated masses at the end of the simulation at the colision (Tunneling Probability: {tunneling_probability}):")
|
| 133 |
+
for j, quark in enumerate(quark_masses.keys()):
|
| 134 |
+
print(f"{quark}: {particle_masses_evolution[j, -1] / GeV_to_J:.4e} GeV")
|
| 135 |
+
|
| 136 |
+
# Save data to JSON file
|
| 137 |
+
data_filename = os.path.join(data_dir, f"big_bang_simulation_data_{tunneling_probability:.2f}.json")
|
| 138 |
+
data = {
|
| 139 |
+
"tunneling_probability": tunneling_probability,
|
| 140 |
+
"particle_masses_evolution": particle_masses_evolution.tolist(),
|
| 141 |
+
"particle_speeds": particle_speeds.tolist(),
|
| 142 |
+
"particle_temperatures": particle_temperatures.tolist(),
|
| 143 |
+
"tunneling_steps": tunneling_steps.tolist()
|
| 144 |
+
}
|
| 145 |
+
with open(data_filename, "w") as f:
|
| 146 |
+
json.dump(data, f)
|
simAI.py
ADDED
|
File without changes
|
simAZ.py
ADDED
|
@@ -0,0 +1,171 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
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|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
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|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
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|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
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|
|
|
|
|
|
|
|
|
|
|
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|
|
|
|
|
|
|
|
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|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
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|
|
|
|
|
|
|
|
|
|
|
|
|
|
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|
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|
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|
|
|
|
|
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|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import numpy as np
|
| 2 |
+
import pandas as pd
|
| 3 |
+
import json
|
| 4 |
+
import os
|
| 5 |
+
|
| 6 |
+
# Constants
|
| 7 |
+
c = 299792458 # Speed of light in m/s
|
| 8 |
+
E_mc2 = c**2 # Mass-energy equivalence in J/kg
|
| 9 |
+
TSR = E_mc2 / (1.38e-23) # Temperature to Speed Ratio in K/m/s
|
| 10 |
+
alpha = 1.0 # Proportional constant for TSR
|
| 11 |
+
Q = 2 ** (1 / 12) # Fractal structure parameter
|
| 12 |
+
dark_energy_density = 5.96e-27 # Density of dark energy in kg/m^3
|
| 13 |
+
dark_matter_density = 2.25e-27 # Density of dark matter in kg/m^3
|
| 14 |
+
collision_distance = 1e-10 # Distance for collision detection
|
| 15 |
+
Hubble_constant = 70.0 # km/s/Mpc (approximation)
|
| 16 |
+
Hubble_constant_SI = Hubble_constant * 1000 / 3.086e22 # Convert to SI units (s^-1)
|
| 17 |
+
|
| 18 |
+
# Initial conditions
|
| 19 |
+
temperature_initial = 1.0 # Planck temperature in K
|
| 20 |
+
particle_density_initial = 5.16e96 # Planck density in kg/m^3
|
| 21 |
+
particle_speed_initial = TSR * temperature_initial # Initial speed based on TSR
|
| 22 |
+
|
| 23 |
+
# Simulation time
|
| 24 |
+
t_planck = 5.39e-44 # Planck time in s
|
| 25 |
+
t_simulation = t_planck * 1e5 # Shorter timescale for simulation
|
| 26 |
+
|
| 27 |
+
# Updated particle masses (in GeV)
|
| 28 |
+
particle_masses = {
|
| 29 |
+
"up": 2.3e-3,
|
| 30 |
+
"down": 4.8e-3,
|
| 31 |
+
"charm": 1.28,
|
| 32 |
+
"strange": 0.095,
|
| 33 |
+
"top": 173.0,
|
| 34 |
+
"bottom": 4.18,
|
| 35 |
+
"electron": 5.11e-4,
|
| 36 |
+
"muon": 1.05e-1,
|
| 37 |
+
"tau": 1.78,
|
| 38 |
+
"photon": 0,
|
| 39 |
+
"electron_neutrino": 0, # Neutrinos have very small masses
|
| 40 |
+
"muon_neutrino": 0,
|
| 41 |
+
"tau_neutrino": 0,
|
| 42 |
+
"W_boson": 80.379,
|
| 43 |
+
"Z_boson": 91.1876,
|
| 44 |
+
"Higgs_boson": 125.1,
|
| 45 |
+
"gluon": 0, # Massless
|
| 46 |
+
"proton": 0.938,
|
| 47 |
+
"neutron": 0.939,
|
| 48 |
+
"pion_plus": 0.140,
|
| 49 |
+
"pion_zero": 0.135,
|
| 50 |
+
"kaon_plus": 0.494,
|
| 51 |
+
"kaon_zero": 0.498
|
| 52 |
+
}
|
| 53 |
+
|
| 54 |
+
# Conversion factor from GeV to J
|
| 55 |
+
GeV_to_J = 1.60217662e-10
|
| 56 |
+
|
| 57 |
+
# Simulation setup
|
| 58 |
+
num_steps = int(t_simulation / t_planck)
|
| 59 |
+
|
| 60 |
+
# Tunneling probabilities to investigate
|
| 61 |
+
tunneling_probabilities = np.arange(0.1, 1.5, 0.1) # Exclude 1.0
|
| 62 |
+
|
| 63 |
+
# Create a directory to store the data
|
| 64 |
+
data_dir = "big_bang_simulation_data"
|
| 65 |
+
os.makedirs(data_dir, exist_ok=True)
|
| 66 |
+
|
| 67 |
+
# Functions to incorporate relativistic effects and collisions
|
| 68 |
+
def relativistic_energy(particle_speed, particle_mass):
|
| 69 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 70 |
+
return particle_mass * c**2 / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 71 |
+
|
| 72 |
+
def relativistic_momentum(particle_speed, particle_mass):
|
| 73 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 74 |
+
return particle_mass * particle_speed / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 75 |
+
|
| 76 |
+
def update_speed(current_speed, current_temperature, particle_mass):
|
| 77 |
+
"""Update the speed of a particle based on temperature and mass."""
|
| 78 |
+
return TSR * current_temperature # Update speed using TSR
|
| 79 |
+
|
| 80 |
+
def check_collision(particle_speeds, collision_distance):
|
| 81 |
+
epsilon = 1e-15 # A small value to avoid invalid subtraction
|
| 82 |
+
for j in range(len(particle_speeds)):
|
| 83 |
+
for k in range(j+1, len(particle_speeds)):
|
| 84 |
+
if np.abs(particle_speeds[j] - particle_speeds[k]) < collision_distance + epsilon:
|
| 85 |
+
return True, j, k
|
| 86 |
+
return False, -1, -1
|
| 87 |
+
|
| 88 |
+
def handle_collision(particle_speeds, particle_masses, idx1, idx2):
|
| 89 |
+
"""Handle a collision between two particles."""
|
| 90 |
+
if particle_masses[idx1] == 0 or particle_masses[idx2] == 0:
|
| 91 |
+
# Skip handling collisions involving massless particles
|
| 92 |
+
return
|
| 93 |
+
|
| 94 |
+
p1 = relativistic_momentum(particle_speeds[idx1], particle_masses[idx1])
|
| 95 |
+
p2 = relativistic_momentum(particle_speeds[idx2], particle_masses[idx2])
|
| 96 |
+
|
| 97 |
+
# Calculate velocities after collision using conservation of momentum
|
| 98 |
+
total_momentum = p1 + p2
|
| 99 |
+
total_mass = particle_masses[idx1] + particle_masses[idx2]
|
| 100 |
+
v1_new = (total_momentum / total_mass) * (particle_masses[idx1] / total_mass)
|
| 101 |
+
v2_new = (total_momentum / total_mass) * (particle_masses[idx2] / total_mass)
|
| 102 |
+
|
| 103 |
+
particle_speeds[idx1], particle_speeds[idx2] = v1_new, v2_new
|
| 104 |
+
|
| 105 |
+
# Simulate the Big Bang with Dark Energy, Dark Matter, Tunneling, and Relativistic Effects
|
| 106 |
+
for tunneling_probability in tunneling_probabilities:
|
| 107 |
+
print(f"Simulating for tunneling probability: {tunneling_probability}")
|
| 108 |
+
|
| 109 |
+
# Initialize arrays for simulation
|
| 110 |
+
particle_speeds = np.zeros((len(particle_masses), num_steps)) # 2D array for speeds
|
| 111 |
+
particle_temperatures = np.zeros((len(particle_masses), num_steps)) # 2D array for temperatures
|
| 112 |
+
particle_masses_evolution = np.zeros((len(particle_masses), num_steps)) # 2D array for mass evolution
|
| 113 |
+
tunneling_steps = np.zeros((len(particle_masses), num_steps), dtype=bool) # 2D array for tunneling steps
|
| 114 |
+
particle_momentum = np.zeros((len(particle_masses), num_steps)) # 2D array for momentum
|
| 115 |
+
total_energy = np.zeros(num_steps) # 1D array for total energy of the system
|
| 116 |
+
|
| 117 |
+
# Create an array of masses for each particle
|
| 118 |
+
particle_masses_array = np.array([mass * GeV_to_J for mass in particle_masses.values()])
|
| 119 |
+
|
| 120 |
+
for j, (particle, mass) in enumerate(particle_masses.items()):
|
| 121 |
+
particle_masses_evolution[j, 0] = particle_masses_array[j] # Initialize mass
|
| 122 |
+
particle_speeds[j, 0] = particle_speed_initial # Initialize speed
|
| 123 |
+
particle_temperatures[j, 0] = temperature_initial # Initialize temperature
|
| 124 |
+
particle_momentum[j, 0] = relativistic_momentum(particle_speeds[j, 0], particle_masses_array[j]) # Initialize momentum
|
| 125 |
+
|
| 126 |
+
for i in range(1, num_steps):
|
| 127 |
+
# Update temperature based on expansion of the universe
|
| 128 |
+
particle_temperatures[j, i] = particle_temperatures[j, i-1] * (1 - Hubble_constant_SI * t_planck)
|
| 129 |
+
|
| 130 |
+
# Update speed using TSR
|
| 131 |
+
particle_speeds[j, i] = update_speed(particle_speeds[j, i-1], particle_temperatures[j, i], particle_masses_array[j])
|
| 132 |
+
|
| 133 |
+
# Apply tunneling effect
|
| 134 |
+
if np.random.rand() < tunneling_probability:
|
| 135 |
+
particle_speeds[j, i] = particle_speeds[j, 0]
|
| 136 |
+
tunneling_steps[j, i] = True
|
| 137 |
+
|
| 138 |
+
# Update mass based on energy conversion
|
| 139 |
+
energy_diff = relativistic_energy(particle_speeds[j, i], particle_masses_array[j]) - relativistic_energy(particle_speeds[j, i - 1], particle_masses_array[j])
|
| 140 |
+
particle_masses_evolution[j, i] = particle_masses_evolution[j, i - 1] + energy_diff / c**2
|
| 141 |
+
|
| 142 |
+
# Check for collisions and handle them
|
| 143 |
+
collision, idx1, idx2 = check_collision(particle_speeds[:, i], collision_distance)
|
| 144 |
+
if collision:
|
| 145 |
+
handle_collision(particle_speeds[:, i], particle_masses_array, idx1, idx2)
|
| 146 |
+
|
| 147 |
+
# Update momentum
|
| 148 |
+
particle_momentum[j, i] = relativistic_momentum(particle_speeds[j, i], particle_masses_array[j])
|
| 149 |
+
|
| 150 |
+
# Update total energy
|
| 151 |
+
total_energy[i] = np.sum([relativistic_energy(particle_speeds[k, i], particle_masses_array[k]) for k in range(len(particle_masses))])
|
| 152 |
+
|
| 153 |
+
# Print calculated masses at the end of the simulation
|
| 154 |
+
print(f"Calculated masses at the end of the simulation (Tunneling Probability: {tunneling_probability}):")
|
| 155 |
+
for j, particle in enumerate(particle_masses.keys()):
|
| 156 |
+
print(f"{particle}: {particle_masses_evolution[j, -1] / GeV_to_J:.4e} GeV")
|
| 157 |
+
|
| 158 |
+
# Save data to JSON file
|
| 159 |
+
data_filename = os.path.join(data_dir, f"big_bang_simulation_data_{tunneling_probability:.2f}.json")
|
| 160 |
+
data = {
|
| 161 |
+
"tunneling_probability": tunneling_probability,
|
| 162 |
+
"particle_masses_evolution": particle_masses_evolution.tolist(),
|
| 163 |
+
"particle_speeds": particle_speeds.tolist(),
|
| 164 |
+
"particle_temperatures": particle_temperatures.tolist(),
|
| 165 |
+
"tunneling_steps": tunneling_steps.tolist(),
|
| 166 |
+
"particle_momentum": particle_momentum.tolist(),
|
| 167 |
+
"total_energy": total_energy.tolist()
|
| 168 |
+
}
|
| 169 |
+
with open(data_filename, "w") as f:
|
| 170 |
+
json.dump(data, f)
|
| 171 |
+
|
simB.py
ADDED
|
@@ -0,0 +1,132 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import numpy as np
|
| 2 |
+
import json
|
| 3 |
+
import os
|
| 4 |
+
|
| 5 |
+
# Constants
|
| 6 |
+
c = 299792458 # Speed of light in m/s
|
| 7 |
+
E_mc2 = c**2 # Mass-energy equivalence in J/kg
|
| 8 |
+
dark_energy_density = 5.96e-27 # Density of dark energy in kg/m^3
|
| 9 |
+
collision_distance = 1e-10 # Distance for collision detection
|
| 10 |
+
|
| 11 |
+
# Initial conditions
|
| 12 |
+
temperature_initial = 1.42e32 # Planck temperature in K
|
| 13 |
+
particle_speed_initial = c # Initially at the speed of light
|
| 14 |
+
|
| 15 |
+
# Simulation time
|
| 16 |
+
t_planck = 5.39e-44 # Planck time in s
|
| 17 |
+
t_simulation = t_planck * 1e5 # Shorter timescale for simulation
|
| 18 |
+
|
| 19 |
+
# Quark masses (in GeV)
|
| 20 |
+
quark_masses = {
|
| 21 |
+
"up": 2.3e-3,
|
| 22 |
+
"down": 4.8e-3,
|
| 23 |
+
"charm": 1.28,
|
| 24 |
+
"strange": 0.095,
|
| 25 |
+
"top": 173.0,
|
| 26 |
+
"bottom": 4.18,
|
| 27 |
+
"electron": 5.11e-4,
|
| 28 |
+
"muon": 1.05e-1,
|
| 29 |
+
"tau": 1.78,
|
| 30 |
+
"photon": 0,
|
| 31 |
+
}
|
| 32 |
+
|
| 33 |
+
# Conversion factor from GeV to J
|
| 34 |
+
GeV_to_J = 1.60217662e-10
|
| 35 |
+
|
| 36 |
+
# Simulation setup
|
| 37 |
+
num_steps = int(t_simulation / t_planck)
|
| 38 |
+
|
| 39 |
+
# Create a directory to store the data
|
| 40 |
+
data_dir = "big_bang_simulation_data"
|
| 41 |
+
os.makedirs(data_dir, exist_ok=True)
|
| 42 |
+
|
| 43 |
+
# Functions to incorporate relativistic effects and collisions
|
| 44 |
+
def relativistic_momentum(particle_speed, particle_mass):
|
| 45 |
+
if particle_speed >= c:
|
| 46 |
+
return np.inf
|
| 47 |
+
return (
|
| 48 |
+
particle_mass
|
| 49 |
+
* particle_speed
|
| 50 |
+
/ np.sqrt(max(1e-10, 1 - (particle_speed / c) ** 2))
|
| 51 |
+
)
|
| 52 |
+
|
| 53 |
+
def update_speed(current_speed, current_temperature, particle_mass):
|
| 54 |
+
# Placeholder for speed update logic
|
| 55 |
+
return current_speed # This should be replaced with actual logic
|
| 56 |
+
|
| 57 |
+
def check_collision(particle_speeds, collision_distance):
|
| 58 |
+
for j in range(len(particle_speeds)):
|
| 59 |
+
for k in range(j + 1, len(particle_speeds)):
|
| 60 |
+
if np.abs(particle_speeds[j] - particle_speeds[k]) < collision_distance:
|
| 61 |
+
return True, j, k
|
| 62 |
+
return False, -1, -1
|
| 63 |
+
|
| 64 |
+
def handle_collision(particle_speeds, idx1, idx2):
|
| 65 |
+
# Exchange momentum for a simplified collision response
|
| 66 |
+
p1 = relativistic_momentum(particle_speeds[idx1], particle_masses[idx1])
|
| 67 |
+
p2 = relativistic_momentum(particle_speeds[idx2], particle_masses[idx2])
|
| 68 |
+
|
| 69 |
+
# Simplified exchange of speeds based on momentum
|
| 70 |
+
particle_speeds[idx1] = p2 / particle_masses[idx1] # Update speed of particle 1
|
| 71 |
+
particle_speeds[idx2] = p1 / particle_masses[idx2] # Update speed of particle 2
|
| 72 |
+
|
| 73 |
+
# Simulate the Big Bang with Dark Energy, Dark Matter, Tunneling, and Relativistic Effects
|
| 74 |
+
for tunneling_probability in np.arange(0.01, 2.5, 0.1):
|
| 75 |
+
print(f"Simulating for tunneling probability: {tunneling_probability}")
|
| 76 |
+
|
| 77 |
+
# Initialize arrays for simulation
|
| 78 |
+
particle_speeds = np.zeros((len(quark_masses), num_steps)) # 2D array for speeds
|
| 79 |
+
particle_temperatures = np.zeros((len(quark_masses), num_steps)) # 2D array for temperatures
|
| 80 |
+
np.zeros((len(quark_masses), num_steps)) # 2D array for temperatures
|
| 81 |
+
particle_masses_evolution = np.zeros((len(quark_masses), num_steps)) # 2D array for mass evolution
|
| 82 |
+
tunneling_steps = np.zeros((len(quark_masses), num_steps), dtype=bool) # 2D array for tunneling steps
|
| 83 |
+
|
| 84 |
+
# Create an array of masses for each quark
|
| 85 |
+
particle_masses = np.array([mass * GeV_to_J for mass in quark_masses.values()])
|
| 86 |
+
|
| 87 |
+
for j, (quark, mass) in enumerate(quark_masses.items()):
|
| 88 |
+
# Initialize particle speeds and temperatures
|
| 89 |
+
particle_speeds[j, 0] = particle_speed_initial
|
| 90 |
+
particle_temperatures[j, 0] = temperature_initial
|
| 91 |
+
particle_masses_evolution[j, 0] = mass * GeV_to_J # Convert to Joules
|
| 92 |
+
|
| 93 |
+
# Time evolution loop
|
| 94 |
+
for step in range(1, num_steps):
|
| 95 |
+
for j in range(len(quark_masses)):
|
| 96 |
+
# Update temperature based on some model (placeholder)
|
| 97 |
+
particle_temperatures[j, step] = particle_temperatures[j, step - 1] * 0.99 # Cooling down
|
| 98 |
+
|
| 99 |
+
# Update speed based on temperature and mass
|
| 100 |
+
particle_speeds[j, step] = update_speed(
|
| 101 |
+
particle_speeds[j, step - 1],
|
| 102 |
+
particle_temperatures[j, step],
|
| 103 |
+
particle_masses[j]
|
| 104 |
+
)
|
| 105 |
+
|
| 106 |
+
# Check for collisions
|
| 107 |
+
collision_detected, idx1, idx2 = check_collision(particle_speeds[:, step], collision_distance)
|
| 108 |
+
if collision_detected:
|
| 109 |
+
handle_collision(particle_speeds[:, step], idx1, idx2)
|
| 110 |
+
|
| 111 |
+
# Tunneling effect (placeholder for actual physics)
|
| 112 |
+
if np.random.rand() < tunneling_probability:
|
| 113 |
+
tunneling_steps[j, step] = True
|
| 114 |
+
# Modify mass or speed based on tunneling (placeholder)
|
| 115 |
+
particle_masses[j] *= 1.1 # Increase mass as an example
|
| 116 |
+
|
| 117 |
+
# Store mass evolution
|
| 118 |
+
particle_masses_evolution[:, step] = particle_masses
|
| 119 |
+
|
| 120 |
+
# Save the simulation data for this tunneling probability
|
| 121 |
+
simulation_data = {
|
| 122 |
+
"particle_speeds": particle_speeds.tolist(), # Convert to list for JSON serialization
|
| 123 |
+
"particle_temperatures": particle_temperatures.tolist(), # Convert to list for JSON serialization
|
| 124 |
+
"particle_masses_evolution": particle_masses_evolution.tolist(), # Convert to list for JSON serialization
|
| 125 |
+
"tunneling_steps": tunneling_steps.tolist(), # Convert to list for JSON serialization
|
| 126 |
+
}
|
| 127 |
+
|
| 128 |
+
with open(os.path.join(data_dir, f"simulation_tunneling_{tunneling_probability:.2f}.json"), "w") as f:
|
| 129 |
+
json.dump(simulation_data, f)
|
| 130 |
+
|
| 131 |
+
print("Simulation completed and data saved.")
|
| 132 |
+
|
simC.py
ADDED
|
@@ -0,0 +1,156 @@
|
|
|
|
|
|
|
|
|
|
|
|
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|
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|
|
|
|
|
|
|
|
|
|
|
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|
|
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|
|
|
|
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|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import numpy as np
|
| 2 |
+
import pandas as pd
|
| 3 |
+
import json
|
| 4 |
+
import os
|
| 5 |
+
|
| 6 |
+
# Constants
|
| 7 |
+
c = 299792458 # Speed of light in m/s
|
| 8 |
+
E_mc2 = c**2 # Mass-energy equivalence in J/kg
|
| 9 |
+
TSR = E_mc2 / (1.38e-23) # Temperature to Speed Ratio in K/m/s
|
| 10 |
+
alpha = 1.0 # Proportional constant for TSR
|
| 11 |
+
Q = 2 ** (1 / 12) # Fractal structure parameter
|
| 12 |
+
dark_energy_density = 5.96e-27 # Density of dark energy in kg/m^3
|
| 13 |
+
dark_matter_density = 2.25e-27 # Density of dark matter in kg/m^3
|
| 14 |
+
collision_distance = 1e-10 # Distance for collision detection
|
| 15 |
+
Hubble_constant = 70.0 # km/s/Mpc (approximation)
|
| 16 |
+
Hubble_constant_SI = Hubble_constant * 1000 / 3.086e22 # Convert to SI units (s^-1)
|
| 17 |
+
|
| 18 |
+
# Initial conditions
|
| 19 |
+
temperature_initial = 1.0 # Planck temperature in K
|
| 20 |
+
particle_density_initial = 5.16e96 # Planck density in kg/m^3
|
| 21 |
+
particle_speed_initial = TSR * temperature_initial # Initial speed based on TSR
|
| 22 |
+
|
| 23 |
+
# Simulation time
|
| 24 |
+
t_planck = 5.39e-44 # Planck time in s
|
| 25 |
+
t_simulation = t_planck * 1e5 # Shorter timescale for simulation
|
| 26 |
+
|
| 27 |
+
# Particle masses (in GeV)
|
| 28 |
+
particle_masses = {
|
| 29 |
+
"up": 2.3e-3,
|
| 30 |
+
"down": 4.8e-3,
|
| 31 |
+
"charm": 1.28,
|
| 32 |
+
"strange": 0.095,
|
| 33 |
+
"top": 173.0,
|
| 34 |
+
"bottom": 4.18,
|
| 35 |
+
"electron": 5.11e-4,
|
| 36 |
+
"muon": 1.05e-1,
|
| 37 |
+
"tau": 1.78,
|
| 38 |
+
"photon": 0,
|
| 39 |
+
"electron_neutrino": 0, # Neutrinos have very small masses
|
| 40 |
+
"muon_neutrino": 0,
|
| 41 |
+
"tau_neutrino": 0,
|
| 42 |
+
"W_boson": 80.379,
|
| 43 |
+
"Z_boson": 91.1876,
|
| 44 |
+
"Higgs_boson": 125.1,
|
| 45 |
+
"gluon": 0, # Massless
|
| 46 |
+
"proton": 0.938,
|
| 47 |
+
"neutron": 0.939,
|
| 48 |
+
"pion_plus": 0.140,
|
| 49 |
+
"pion_zero": 0.135,
|
| 50 |
+
"kaon_plus": 0.494,
|
| 51 |
+
"kaon_zero": 0.498
|
| 52 |
+
}
|
| 53 |
+
|
| 54 |
+
# Conversion factor from GeV to J
|
| 55 |
+
GeV_to_J = 1.60217662e-10
|
| 56 |
+
|
| 57 |
+
# Simulation setup
|
| 58 |
+
num_steps = int(t_simulation / t_planck)
|
| 59 |
+
|
| 60 |
+
# Tunneling probabilities to investigate
|
| 61 |
+
tunneling_probabilities = np.arange(0.001, 1.5, 0.001) # Exclude 1.0
|
| 62 |
+
|
| 63 |
+
# Create a directory to store the data
|
| 64 |
+
data_dir = "big_bang_simulation_data"
|
| 65 |
+
os.makedirs(data_dir, exist_ok=True)
|
| 66 |
+
|
| 67 |
+
# Functions to incorporate relativistic effects and collisions
|
| 68 |
+
def relativistic_energy(particle_speed, particle_mass):
|
| 69 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 70 |
+
return particle_mass * c**2 / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 71 |
+
|
| 72 |
+
def relativistic_momentum(particle_speed, particle_mass):
|
| 73 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 74 |
+
return particle_mass * particle_speed / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 75 |
+
|
| 76 |
+
def update_speed(current_speed, current_temperature, particle_mass):
|
| 77 |
+
"""Update the speed of a particle based on temperature and mass."""
|
| 78 |
+
return TSR * current_temperature # Update speed using TSR
|
| 79 |
+
|
| 80 |
+
def check_collision(particle_speeds, collision_distance, current_step):
|
| 81 |
+
for j in range(len(particle_speeds)):
|
| 82 |
+
for k in range(j+1, len(particle_speeds)):
|
| 83 |
+
if np.abs(particle_speeds[j][current_step] - particle_speeds[k][current_step]) < collision_distance:
|
| 84 |
+
return True, j, k
|
| 85 |
+
return False, -1, -1
|
| 86 |
+
|
| 87 |
+
def handle_collision(particle_speeds, particle_masses, idx1, idx2, current_step):
|
| 88 |
+
"""Handle a collision between two particles."""
|
| 89 |
+
p1 = relativistic_momentum(particle_speeds[idx1][current_step], particle_masses[idx1])
|
| 90 |
+
p2 = relativistic_momentum(particle_speeds[idx2][current_step], particle_masses[idx2])
|
| 91 |
+
|
| 92 |
+
# Calculate velocities after collision using conservation of momentum
|
| 93 |
+
total_momentum = p1 + p2
|
| 94 |
+
total_mass = particle_masses[idx1] + particle_masses[idx2]
|
| 95 |
+
v1_new = (total_momentum / total_mass) * (particle_masses[idx1] / total_mass)
|
| 96 |
+
v2_new = (total_momentum / total_mass) * (particle_masses[idx2] / total_mass)
|
| 97 |
+
|
| 98 |
+
particle_speeds[idx1][current_step] = v1_new
|
| 99 |
+
particle_speeds[idx2][current_step] = v2_new
|
| 100 |
+
|
| 101 |
+
# Simulate the Big Bang with Dark Energy, Dark Matter, Tunneling, and Relativistic Effects
|
| 102 |
+
for tunneling_probability in tunneling_probabilities:
|
| 103 |
+
print(f"Simulating for tunneling probability: {tunneling_probability}")
|
| 104 |
+
|
| 105 |
+
# Initialize arrays for simulation
|
| 106 |
+
num_particles = len(particle_masses)
|
| 107 |
+
particle_speeds = [[particle_speed_initial] * num_steps for _ in range(num_particles)]
|
| 108 |
+
particle_temperatures = [[temperature_initial] * num_steps for _ in range(num_particles)]
|
| 109 |
+
particle_masses_evolution = [[mass * GeV_to_J] * num_steps for mass in particle_masses.values()]
|
| 110 |
+
tunneling_steps = [[False] * num_steps for _ in range(num_particles)]
|
| 111 |
+
particle_masses_array = np.array([mass * GeV_to_J for mass in particle_masses.values()])
|
| 112 |
+
|
| 113 |
+
for current_step in range(1, num_steps):
|
| 114 |
+
for j in range(num_particles):
|
| 115 |
+
# Update temperature based on expansion of the universe
|
| 116 |
+
particle_temperatures[j][current_step] = particle_temperatures[j][current_step-1] * (1 - Hubble_constant_SI * t_planck)
|
| 117 |
+
|
| 118 |
+
# Update speed using TSR
|
| 119 |
+
particle_speeds[j][current_step] = update_speed(particle_speeds[j][current_step-1], particle_temperatures[j][current_step], particle_masses_array[j])
|
| 120 |
+
|
| 121 |
+
# Apply tunneling effect
|
| 122 |
+
if np.random.rand() < tunneling_probability:
|
| 123 |
+
particle_speeds[j][current_step] = particle_speeds[j][0]
|
| 124 |
+
tunneling_steps[j][current_step] = True
|
| 125 |
+
|
| 126 |
+
# Check for collisions
|
| 127 |
+
collision_detected, idx1, idx2 = check_collision(particle_speeds, collision_distance, current_step)
|
| 128 |
+
if collision_detected:
|
| 129 |
+
handle_collision(particle_speeds, particle_masses_array, idx1, idx2, current_step)
|
| 130 |
+
|
| 131 |
+
# Calculate entropy using von Neumann entropy formula
|
| 132 |
+
for j in range(num_particles):
|
| 133 |
+
if particle_masses_array[j] == 0:
|
| 134 |
+
entropy = 0
|
| 135 |
+
else:
|
| 136 |
+
entropy = -particle_masses_array[j] * np.log1p(particle_masses_array[j])
|
| 137 |
+
|
| 138 |
+
# Update mass based on entropy
|
| 139 |
+
particle_masses_evolution[j][current_step] = particle_masses_evolution[j][current_step-1] + entropy / c**2
|
| 140 |
+
|
| 141 |
+
# Print calculated masses at the end of the simulation
|
| 142 |
+
print(f"Calculated masses at the end of the simulation using the von Neumann entropy (Tunneling Probability: {tunneling_probability}):")
|
| 143 |
+
for j, particle in enumerate(particle_masses.keys()):
|
| 144 |
+
print(f"{particle}: {particle_masses_evolution[j][-1] / GeV_to_J:.4e} GeV")
|
| 145 |
+
|
| 146 |
+
# Save data to JSON file
|
| 147 |
+
data_filename = os.path.join(data_dir, f"big_bang_simulation_data_{tunneling_probability:.2f}.json")
|
| 148 |
+
data = {
|
| 149 |
+
"tunneling_probability": tunneling_probability,
|
| 150 |
+
"particle_masses_evolution": particle_masses_evolution, # No need for tolist()
|
| 151 |
+
"particle_speeds": particle_speeds,
|
| 152 |
+
"particle_temperatures": particle_temperatures,
|
| 153 |
+
"tunneling_steps": tunneling_steps
|
| 154 |
+
}
|
| 155 |
+
with open(data_filename, "w") as f:
|
| 156 |
+
json.dump(data, f)
|
simD.py
ADDED
|
@@ -0,0 +1,163 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import numpy as np
|
| 2 |
+
import pandas as pd
|
| 3 |
+
import json
|
| 4 |
+
import os
|
| 5 |
+
|
| 6 |
+
# Constants
|
| 7 |
+
c = 299792458 # Speed of light in m/s
|
| 8 |
+
E_mc2 = c**2 # Mass-energy equivalence in J/kg
|
| 9 |
+
TSR = E_mc2 / (1.38e-23) # Temperature to Speed Ratio in K/m/s
|
| 10 |
+
alpha = 1.0 # Proportional constant for TSR
|
| 11 |
+
Q = 2 ** (1 / 12) # Fractal structure parameter
|
| 12 |
+
dark_energy_density = 5.96e-27 # Density of dark energy in kg/m^3
|
| 13 |
+
dark_matter_density = 2.25e-27 # Density of dark matter in kg/m^3
|
| 14 |
+
collision_distance = 1e-10 # Distance for collision detection
|
| 15 |
+
Hubble_constant = 70.0 # km/s/Mpc (approximation)
|
| 16 |
+
Hubble_constant_SI = Hubble_constant * 1000 / 3.086e22 # Convert to SI units (s^-1)
|
| 17 |
+
|
| 18 |
+
# Initial conditions
|
| 19 |
+
temperature_initial = 1.0 # Planck temperature in K
|
| 20 |
+
particle_density_initial = 5.16e96 # Planck density in kg/m^3
|
| 21 |
+
particle_speed_initial = TSR * temperature_initial # Initial speed based on TSR
|
| 22 |
+
|
| 23 |
+
# Simulation time
|
| 24 |
+
t_planck = 5.39e-44 # Planck time in s
|
| 25 |
+
t_simulation = t_planck * 1e5 # Shorter timescale for simulation
|
| 26 |
+
|
| 27 |
+
# Updated particle masses (in GeV)
|
| 28 |
+
particle_masses = {
|
| 29 |
+
"up": 2.3e-3,
|
| 30 |
+
"down": 4.8e-3,
|
| 31 |
+
"charm": 1.28,
|
| 32 |
+
"strange": 0.095,
|
| 33 |
+
"top": 173.0,
|
| 34 |
+
"bottom": 4.18,
|
| 35 |
+
"electron": 5.11e-4,
|
| 36 |
+
"muon": 1.05e-1,
|
| 37 |
+
"tau": 1.78,
|
| 38 |
+
"photon": 0,
|
| 39 |
+
"electron_neutrino": 0, # Neutrinos have very small masses
|
| 40 |
+
"muon_neutrino": 0,
|
| 41 |
+
"tau_neutrino": 0,
|
| 42 |
+
"W_boson": 80.379,
|
| 43 |
+
"Z_boson": 91.1876,
|
| 44 |
+
"Higgs_boson": 125.1,
|
| 45 |
+
"gluon": 0, # Massless
|
| 46 |
+
"proton": 0.938,
|
| 47 |
+
"neutron": 0.939,
|
| 48 |
+
"pion_plus": 0.140,
|
| 49 |
+
"pion_zero": 0.135,
|
| 50 |
+
"kaon_plus": 0.494,
|
| 51 |
+
"kaon_zero": 0.498
|
| 52 |
+
}
|
| 53 |
+
|
| 54 |
+
# Conversion factor from GeV to J
|
| 55 |
+
GeV_to_J = 1.60217662e-10
|
| 56 |
+
|
| 57 |
+
# Simulation setup
|
| 58 |
+
num_steps = int(t_simulation / t_planck)
|
| 59 |
+
|
| 60 |
+
# Tunneling probabilities to investigate
|
| 61 |
+
tunneling_probabilities = np.arange(0.1, 1.5, 0.1) # Exclude 1.0
|
| 62 |
+
|
| 63 |
+
# Create a directory to store the data
|
| 64 |
+
data_dir = "big_bang_simulation_data"
|
| 65 |
+
os.makedirs(data_dir, exist_ok=True)
|
| 66 |
+
|
| 67 |
+
# Functions to incorporate relativistic effects and collisions
|
| 68 |
+
def relativistic_energy(particle_speed, particle_mass):
|
| 69 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 70 |
+
return particle_mass * c**2 / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 71 |
+
|
| 72 |
+
def relativistic_momentum(particle_speed, particle_mass):
|
| 73 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 74 |
+
return particle_mass * particle_speed / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 75 |
+
|
| 76 |
+
def update_speed(current_speed, current_temperature, particle_mass):
|
| 77 |
+
"""Update the speed of a particle based on temperature and mass."""
|
| 78 |
+
return TSR * current_temperature # Update speed using TSR
|
| 79 |
+
|
| 80 |
+
def check_collision(particle_speeds, collision_distance):
|
| 81 |
+
epsilon = 1e-15 # A small value to avoid invalid subtraction
|
| 82 |
+
for j in range(len(particle_speeds)):
|
| 83 |
+
for k in range(j+1, len(particle_speeds)):
|
| 84 |
+
if np.abs(particle_speeds[j] - particle_speeds[k]) < collision_distance + epsilon:
|
| 85 |
+
return True, j, k
|
| 86 |
+
return False, -1, -1
|
| 87 |
+
|
| 88 |
+
def handle_collision(particle_speeds, particle_masses, idx1, idx2):
|
| 89 |
+
"""Handle a collision between two particles."""
|
| 90 |
+
p1 = relativistic_momentum(particle_speeds[idx1], particle_masses[idx1])
|
| 91 |
+
p2 = relativistic_momentum(particle_speeds[idx2], particle_masses[idx2])
|
| 92 |
+
|
| 93 |
+
# Calculate velocities after collision using conservation of momentum
|
| 94 |
+
total_momentum = p1 + p2
|
| 95 |
+
total_mass = particle_masses[idx1] + particle_masses[idx2]
|
| 96 |
+
|
| 97 |
+
# Check for division by zero
|
| 98 |
+
if total_mass == 0:
|
| 99 |
+
# If total_mass is zero, set the velocities to zero
|
| 100 |
+
particle_speeds[idx1] = 0
|
| 101 |
+
particle_speeds[idx2] = 0
|
| 102 |
+
return
|
| 103 |
+
|
| 104 |
+
v1_new = (total_momentum / total_mass) * (particle_masses[idx1] / total_mass)
|
| 105 |
+
v2_new = (total_momentum / total_mass) * (particle_masses[idx2] / total_mass)
|
| 106 |
+
|
| 107 |
+
particle_speeds[idx1], particle_speeds[idx2] = v1_new, v2_new
|
| 108 |
+
|
| 109 |
+
# Simulate the Big Bang with Dark Energy, Dark Matter, Tunneling, and Relativistic Effects
|
| 110 |
+
for tunneling_probability in tunneling_probabilities:
|
| 111 |
+
print(f"Simulating for tunneling probability: {tunneling_probability}")
|
| 112 |
+
|
| 113 |
+
# Initialize arrays for simulation
|
| 114 |
+
particle_speeds = np.zeros((len(particle_masses), num_steps)) # 2D array for speeds
|
| 115 |
+
particle_temperatures = np.zeros((len(particle_masses), num_steps)) # 2D array for temperatures
|
| 116 |
+
particle_masses_evolution = np.zeros((len(particle_masses), num_steps)) # 2D array for mass evolution
|
| 117 |
+
tunneling_steps = np.zeros((len(particle_masses), num_steps), dtype=bool) # 2D array for tunneling steps
|
| 118 |
+
|
| 119 |
+
# Create an array of masses for each particle
|
| 120 |
+
particle_masses_array = np.array([mass * GeV_to_J for mass in particle_masses.values()])
|
| 121 |
+
|
| 122 |
+
for j, (particle, mass) in enumerate(particle_masses.items()):
|
| 123 |
+
particle_masses_evolution[j, 0] = particle_masses_array[j] # Initialize mass
|
| 124 |
+
particle_speeds[j, 0] = particle_speed_initial # Initialize speed
|
| 125 |
+
particle_temperatures[j, 0] = temperature_initial # Initialize temperature
|
| 126 |
+
|
| 127 |
+
for i in range(1, num_steps):
|
| 128 |
+
# Update temperature based on expansion of the universe
|
| 129 |
+
particle_temperatures[j, i] = particle_temperatures[j, i-1] * (1 - Hubble_constant_SI * t_planck)
|
| 130 |
+
|
| 131 |
+
# Update speed using TSR
|
| 132 |
+
particle_speeds[j, i] = update_speed(particle_speeds[j, i-1], particle_temperatures[j, i], particle_masses_array[j])
|
| 133 |
+
|
| 134 |
+
# Apply tunneling effect
|
| 135 |
+
if np.random.rand() < tunneling_probability:
|
| 136 |
+
particle_speeds[j, i] = particle_speeds[j, 0]
|
| 137 |
+
tunneling_steps[j, i] = True
|
| 138 |
+
|
| 139 |
+
# Update mass based on energy conversion
|
| 140 |
+
energy_diff = relativistic_energy(particle_speeds[j, i], particle_masses_array[j]) - relativistic_energy(particle_speeds[j, i - 1], particle_masses_array[j])
|
| 141 |
+
particle_masses_evolution[j, i] = particle_masses_evolution[j, i - 1] + energy_diff / c**2
|
| 142 |
+
|
| 143 |
+
# Check for collisions and handle them
|
| 144 |
+
collision, idx1, idx2 = check_collision(particle_speeds[:, i], collision_distance)
|
| 145 |
+
if collision:
|
| 146 |
+
handle_collision(particle_speeds[:, i], particle_masses_array, idx1, idx2)
|
| 147 |
+
|
| 148 |
+
# Print calculated masses at the end of the simulation
|
| 149 |
+
print(f"Calculated masses at the end of the simulation at the colision (Tunneling Probability: {tunneling_probability}):")
|
| 150 |
+
for j, particle in enumerate(particle_masses.keys()):
|
| 151 |
+
print(f"{particle}: {particle_masses_evolution[j, -1] / GeV_to_J:.4e} GeV")
|
| 152 |
+
|
| 153 |
+
# Save data to JSON file
|
| 154 |
+
data_filename = os.path.join(data_dir, f"big_bang_simulation_data_{tunneling_probability:.2f}.json")
|
| 155 |
+
data = {
|
| 156 |
+
"tunneling_probability": tunneling_probability,
|
| 157 |
+
"particle_masses_evolution": particle_masses_evolution.tolist(),
|
| 158 |
+
"particle_speeds": particle_speeds.tolist(),
|
| 159 |
+
"particle_temperatures": particle_temperatures.tolist(),
|
| 160 |
+
"tunneling_steps": tunneling_steps.tolist()
|
| 161 |
+
}
|
| 162 |
+
with open(data_filename, "w") as f:
|
| 163 |
+
json.dump(data, f)
|
simE.py
ADDED
|
@@ -0,0 +1,173 @@
|
|
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|
|
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|
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|
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|
|
|
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|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import numpy as np
|
| 2 |
+
import pandas as pd
|
| 3 |
+
import json
|
| 4 |
+
import os
|
| 5 |
+
|
| 6 |
+
# Constants
|
| 7 |
+
c = 299792458 # Speed of light in m/s
|
| 8 |
+
E_mc2 = c**2 # Mass-energy equivalence in J/kg
|
| 9 |
+
TSR = E_mc2 / (1.38e-23) # Temperature to Speed Ratio in K/m/s
|
| 10 |
+
alpha = 1.0 # Proportional constant for TSR
|
| 11 |
+
Q = 2 ** (1 / 12) # Fractal structure parameter
|
| 12 |
+
dark_energy_density = 5.96e-27 # Density of dark energy in kg/m^3
|
| 13 |
+
dark_matter_density = 2.25e-27 # Density of dark matter in kg/m^3
|
| 14 |
+
collision_distance = 1e-10 # Distance for collision detection
|
| 15 |
+
Hubble_constant = 70.0 # km/s/Mpc (approximation)
|
| 16 |
+
Hubble_constant_SI = Hubble_constant * 1000 / 3.086e22 # Convert to SI units (s^-1)
|
| 17 |
+
|
| 18 |
+
# Initial conditions
|
| 19 |
+
temperature_initial = 1.0 # Planck temperature in K
|
| 20 |
+
particle_density_initial = 5.16e96 # Planck density in kg/m^3
|
| 21 |
+
particle_speed_initial = TSR * temperature_initial # Initial speed based on TSR
|
| 22 |
+
|
| 23 |
+
# Simulation time
|
| 24 |
+
t_planck = 5.39e-44 # Planck time in s
|
| 25 |
+
t_simulation = t_planck * 1e5 # Shorter timescale for simulation
|
| 26 |
+
|
| 27 |
+
# Updated particle masses (in GeV)
|
| 28 |
+
particle_masses = {
|
| 29 |
+
"up": 2.3e-3,
|
| 30 |
+
"down": 4.8e-3,
|
| 31 |
+
"charm": 1.28,
|
| 32 |
+
"strange": 0.095,
|
| 33 |
+
"top": 173.0,
|
| 34 |
+
"bottom": 4.18,
|
| 35 |
+
"electron": 5.11e-4,
|
| 36 |
+
"muon": 1.05e-1,
|
| 37 |
+
"tau": 1.78,
|
| 38 |
+
"photon": 0,
|
| 39 |
+
"electron_neutrino": 0, # Neutrinos have very small masses
|
| 40 |
+
"muon_neutrino": 0,
|
| 41 |
+
"tau_neutrino": 0,
|
| 42 |
+
"W_boson": 80.379,
|
| 43 |
+
"Z_boson": 91.1876,
|
| 44 |
+
"Higgs_boson": 125.1,
|
| 45 |
+
"gluon": 0, # Massless
|
| 46 |
+
"proton": 0.938,
|
| 47 |
+
"neutron": 0.939,
|
| 48 |
+
"pion_plus": 0.140,
|
| 49 |
+
"pion_zero": 0.135,
|
| 50 |
+
"kaon_plus": 0.494,
|
| 51 |
+
"kaon_zero": 0.498
|
| 52 |
+
}
|
| 53 |
+
|
| 54 |
+
# Conversion factor from GeV to J
|
| 55 |
+
GeV_to_J = 1.60217662e-10
|
| 56 |
+
|
| 57 |
+
# Simulation setup
|
| 58 |
+
num_steps = int(t_simulation / t_planck)
|
| 59 |
+
|
| 60 |
+
# Tunneling probabilities to investigate
|
| 61 |
+
tunneling_probabilities = np.arange(0.1, 1.5, 0.1) # Exclude 1.0
|
| 62 |
+
|
| 63 |
+
# Create a directory to store the data
|
| 64 |
+
data_dir = "big_bang_simulation_data"
|
| 65 |
+
os.makedirs(data_dir, exist_ok=True)
|
| 66 |
+
|
| 67 |
+
# Functions to incorporate relativistic effects and collisions
|
| 68 |
+
def relativistic_energy(particle_speed, particle_mass):
|
| 69 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 70 |
+
return particle_mass * c**2 / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 71 |
+
|
| 72 |
+
def relativistic_momentum(particle_speed, particle_mass):
|
| 73 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 74 |
+
return particle_mass * particle_speed / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 75 |
+
|
| 76 |
+
def update_speed(current_speed, current_temperature, particle_mass):
|
| 77 |
+
"""Update the speed of a particle based on temperature and mass."""
|
| 78 |
+
return TSR * current_temperature # Update speed using TSR
|
| 79 |
+
|
| 80 |
+
def check_collision(particle_speeds, collision_distance):
|
| 81 |
+
epsilon = 1e-15 # A small value to avoid invalid subtraction
|
| 82 |
+
for j in range(len(particle_speeds)):
|
| 83 |
+
for k in range(j+1, len(particle_speeds)):
|
| 84 |
+
if np.abs(particle_speeds[j] - particle_speeds[k]) < collision_distance + epsilon:
|
| 85 |
+
return True, j, k
|
| 86 |
+
return False, -1, -1
|
| 87 |
+
|
| 88 |
+
def handle_collision(particle_speeds, particle_masses, idx1, idx2, current_step):
|
| 89 |
+
"""Handle a collision between two particles."""
|
| 90 |
+
if particle_masses[idx1] == 0 or particle_masses[idx2] == 0:
|
| 91 |
+
# Skip handling collisions involving massless particles
|
| 92 |
+
return
|
| 93 |
+
|
| 94 |
+
p1 = relativistic_momentum(particle_speeds[idx1, current_step], particle_masses[idx1])
|
| 95 |
+
p2 = relativistic_momentum(particle_speeds[idx2, current_step], particle_masses[idx2])
|
| 96 |
+
|
| 97 |
+
# Calculate velocities after collision using conservation of momentum
|
| 98 |
+
total_momentum = p1 + p2
|
| 99 |
+
total_mass = particle_masses[idx1] + particle_masses[idx2]
|
| 100 |
+
v1_new = (total_momentum / total_mass) * (particle_masses[idx1] / total_mass)
|
| 101 |
+
v2_new = (total_momentum / total_mass) * (particle_masses[idx2] / total_mass)
|
| 102 |
+
|
| 103 |
+
particle_speeds[idx1, current_step], particle_speeds[idx2, current_step] = v1_new, v2_new
|
| 104 |
+
|
| 105 |
+
|
| 106 |
+
# Simulate the Big Bang with Dark Energy, Dark Matter, Tunneling, Relativistic Effects, Redshift, and Entanglement
|
| 107 |
+
for tunneling_probability in tunneling_probabilities:
|
| 108 |
+
print(f"Simulating for tunneling probability: {tunneling_probability}")
|
| 109 |
+
|
| 110 |
+
# Initialize arrays for simulation
|
| 111 |
+
num_particles = len(particle_masses)
|
| 112 |
+
particle_speeds = np.zeros((num_particles, num_steps)) # 2D array for speeds
|
| 113 |
+
particle_temperatures = np.zeros((num_particles, num_steps)) # 2D array for temperatures
|
| 114 |
+
particle_masses_evolution = np.zeros((num_particles, num_steps)) # 2D array for mass evolution
|
| 115 |
+
tunneling_steps = np.zeros((num_particles, num_steps), dtype=bool) # 2D array for tunneling steps
|
| 116 |
+
particle_momentum = np.zeros((num_particles, num_steps)) # 2D array for momentum
|
| 117 |
+
total_energy = np.zeros(num_steps) # 1D array for total energy of the system
|
| 118 |
+
redshifts = np.zeros((num_particles, num_steps)) # 2D array for redshift
|
| 119 |
+
entanglement_entropies = np.zeros((num_particles, num_steps)) # 2D array for entanglement entropy
|
| 120 |
+
particle_states = np.random.rand(num_particles, num_steps) # Placeholder for particle states
|
| 121 |
+
|
| 122 |
+
# Create an array of masses for each particle
|
| 123 |
+
particle_masses_array = np.array([mass * GeV_to_J for mass in particle_masses.values()])
|
| 124 |
+
|
| 125 |
+
for j, (particle, mass) in enumerate(particle_masses.items()):
|
| 126 |
+
particle_speeds[j, 0] = particle_speed_initial # Initialize speed
|
| 127 |
+
particle_masses_evolution[j, 0] = mass * GeV_to_J # Initialize mass evolution
|
| 128 |
+
|
| 129 |
+
for current_step in range(1, num_steps):
|
| 130 |
+
for j in range(num_particles):
|
| 131 |
+
# Update temperature based on expansion of the universe
|
| 132 |
+
particle_temperatures[j, current_step] = particle_temperatures[j, current_step-1] * (1 - Hubble_constant_SI * t_planck)
|
| 133 |
+
|
| 134 |
+
# Update speed using TSR
|
| 135 |
+
particle_speeds[j, current_step] = update_speed(particle_speeds[j, current_step-1], particle_temperatures[j, current_step], particle_masses_array[j])
|
| 136 |
+
|
| 137 |
+
# Apply tunneling effect
|
| 138 |
+
if np.random.rand() < tunneling_probability:
|
| 139 |
+
particle_speeds[j, current_step] = particle_speeds[j, 0]
|
| 140 |
+
tunneling_steps[j, current_step] = True
|
| 141 |
+
|
| 142 |
+
# Calculate redshift
|
| 143 |
+
redshifts[j, current_step] = (1 + particle_speeds[j, current_step] / c)
|
| 144 |
+
|
| 145 |
+
# Calculate entanglement entropy
|
| 146 |
+
entanglement_entropies[j, current_step] = -np.sum(particle_states[j, current_step] * np.log(particle_states[j, current_step]))
|
| 147 |
+
|
| 148 |
+
# Update mass evolution
|
| 149 |
+
particle_masses_evolution[j, current_step] = particle_masses_evolution[j, current_step-1] * (1 - dark_energy_density * t_planck)
|
| 150 |
+
|
| 151 |
+
# Check for collisions
|
| 152 |
+
collision_detected, idx1, idx2 = check_collision(particle_speeds[:, current_step], collision_distance)
|
| 153 |
+
if collision_detected:
|
| 154 |
+
handle_collision(particle_speeds, particle_masses_array, idx1, idx2, current_step)
|
| 155 |
+
|
| 156 |
+
# Print calculated masses at the end of the simulation
|
| 157 |
+
print(f"Calculated masses at the end of the simulation (Tunneling Probability: {tunneling_probability}):")
|
| 158 |
+
for j, particle in enumerate(particle_masses.keys()):
|
| 159 |
+
print(f"{particle}: {particle_masses_evolution[j, -1] / GeV_to_J:.4e} GeV")
|
| 160 |
+
|
| 161 |
+
# Save data to JSON file
|
| 162 |
+
data_filename = os.path.join(data_dir, f"big_bang_simulation_data_{tunneling_probability:.2f}.json")
|
| 163 |
+
data = {
|
| 164 |
+
"tunneling_probability": tunneling_probability,
|
| 165 |
+
"particle_masses_evolution": particle_masses_evolution.tolist(),
|
| 166 |
+
"particle_speeds": particle_speeds.tolist(),
|
| 167 |
+
"particle_temperatures": particle_temperatures.tolist(),
|
| 168 |
+
"tunneling_steps": tunneling_steps.tolist(),
|
| 169 |
+
"redshifts": redshifts.tolist(),
|
| 170 |
+
"entanglement_entropies": entanglement_entropies.tolist()
|
| 171 |
+
}
|
| 172 |
+
with open(data_filename, "w") as f:
|
| 173 |
+
json.dump(data, f)
|
simZ.py
ADDED
|
@@ -0,0 +1,142 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import numpy as np
|
| 2 |
+
import pandas as pd
|
| 3 |
+
import json
|
| 4 |
+
import os
|
| 5 |
+
|
| 6 |
+
# Constants
|
| 7 |
+
c = 299792458 # Speed of light in m/s
|
| 8 |
+
E_mc2 = c**2 # Mass-energy equivalence in J/kg
|
| 9 |
+
TSR = E_mc2 / (1.38e-23) # Temperature to Speed Ratio in K/m/s
|
| 10 |
+
alpha = 1.0 # Proportional constant for TSR
|
| 11 |
+
Q = 2 ** (1 / 12) # Fractal structure parameter
|
| 12 |
+
dark_energy_density = 5.96e-27 # Density of dark energy in kg/m^3
|
| 13 |
+
dark_matter_density = 2.25e-27 # Density of dark matter in kg/m^3
|
| 14 |
+
collision_distance = 1e-10 # Distance for collision detection
|
| 15 |
+
Hubble_constant = 70.0 # km/s/Mpc (approximation)
|
| 16 |
+
Hubble_constant_SI = Hubble_constant * 1000 / 3.086e22 # Convert to SI units (s^-1)
|
| 17 |
+
|
| 18 |
+
# Initial conditions
|
| 19 |
+
temperature_initial = 1.0 # Planck temperature in K
|
| 20 |
+
particle_density_initial = 5.16e96 # Planck density in kg/m^3
|
| 21 |
+
particle_speed_initial = TSR * temperature_initial # Initial speed based on TSR
|
| 22 |
+
|
| 23 |
+
# Simulation time
|
| 24 |
+
t_planck = 5.39e-44 # Planck time in s
|
| 25 |
+
t_simulation = t_planck * 1e5 # Shorter timescale for simulation
|
| 26 |
+
|
| 27 |
+
# Quark masses (in GeV) - used for initial mass values and comparison
|
| 28 |
+
quark_masses = {
|
| 29 |
+
"up": 2.3e-3,
|
| 30 |
+
"down": 4.8e-3,
|
| 31 |
+
"charm": 1.28,
|
| 32 |
+
"strange": 0.095,
|
| 33 |
+
"top": 173.0,
|
| 34 |
+
"bottom": 4.18,
|
| 35 |
+
"electron": 5.11e-4,
|
| 36 |
+
"muon": 1.05e-1,
|
| 37 |
+
"tau": 1.78,
|
| 38 |
+
"photon": 0,
|
| 39 |
+
}
|
| 40 |
+
|
| 41 |
+
# Conversion factor from GeV to J
|
| 42 |
+
GeV_to_J = 1.60217662e-10
|
| 43 |
+
|
| 44 |
+
# Simulation setup
|
| 45 |
+
num_steps = int(t_simulation / t_planck)
|
| 46 |
+
|
| 47 |
+
# Tunneling probabilities to investigate
|
| 48 |
+
tunneling_probabilities = np.arange(0.1, 1.5, 0.1) # Exclude 1.0
|
| 49 |
+
|
| 50 |
+
# Create a directory to store the data
|
| 51 |
+
data_dir = "big_bang_simulation_data"
|
| 52 |
+
os.makedirs(data_dir, exist_ok=True)
|
| 53 |
+
|
| 54 |
+
# Functions to incorporate relativistic effects and collisions
|
| 55 |
+
def relativistic_energy(particle_speed, particle_mass):
|
| 56 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 57 |
+
return particle_mass * c**2 / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 58 |
+
|
| 59 |
+
def relativistic_momentum(particle_speed, particle_mass):
|
| 60 |
+
epsilon = 1e-15 # A small value to avoid division by zero
|
| 61 |
+
return particle_mass * particle_speed / np.sqrt(max(1e-15, 1 - (particle_speed / c) ** 2 + epsilon))
|
| 62 |
+
|
| 63 |
+
def update_speed(current_speed, current_temperature, particle_mass):
|
| 64 |
+
"""Update the speed of a particle based on temperature and mass."""
|
| 65 |
+
return TSR * current_temperature # Update speed using TSR
|
| 66 |
+
|
| 67 |
+
def check_collision(particle_speeds, collision_distance):
|
| 68 |
+
epsilon = 1e-15 # A small value to avoid invalid subtraction
|
| 69 |
+
for j in range(len(particle_speeds)):
|
| 70 |
+
for k in range(j+1, len(particle_speeds)):
|
| 71 |
+
if np.abs(particle_speeds[j] - particle_speeds[k]) < collision_distance + epsilon:
|
| 72 |
+
return True, j, k
|
| 73 |
+
return False, -1, -1
|
| 74 |
+
|
| 75 |
+
def handle_collision(particle_speeds, particle_masses, idx1, idx2):
|
| 76 |
+
"""Handle a collision between two particles."""
|
| 77 |
+
p1 = relativistic_momentum(particle_speeds[idx1], particle_masses[idx1])
|
| 78 |
+
p2 = relativistic_momentum(particle_speeds[idx2], particle_masses[idx2])
|
| 79 |
+
|
| 80 |
+
# Calculate velocities after collision using conservation of momentum
|
| 81 |
+
total_momentum = p1 + p2
|
| 82 |
+
total_mass = particle_masses[idx1] + particle_masses[idx2]
|
| 83 |
+
v1_new = (total_momentum / total_mass) * (particle_masses[idx1] / total_mass)
|
| 84 |
+
v2_new = (total_momentum / total_mass) * (particle_masses[idx2] / total_mass)
|
| 85 |
+
|
| 86 |
+
particle_speeds[idx1], particle_speeds[idx2] = v1_new, v2_new
|
| 87 |
+
|
| 88 |
+
# Simulate the Big Bang with Dark Energy, Dark Matter, Tunneling, and Relativistic Effects
|
| 89 |
+
for tunneling_probability in tunneling_probabilities:
|
| 90 |
+
print(f"Simulating for tunneling probability: {tunneling_probability}")
|
| 91 |
+
|
| 92 |
+
# Initialize arrays for simulation
|
| 93 |
+
particle_speeds = np.zeros((len(quark_masses), num_steps)) # 2D array for speeds
|
| 94 |
+
particle_temperatures = np.zeros((len(quark_masses), num_steps)) # 2D array for temperatures
|
| 95 |
+
particle_masses_evolution = np.zeros((len(quark_masses), num_steps)) # 2D array for mass evolution
|
| 96 |
+
tunneling_steps = np.zeros((len(quark_masses), num_steps), dtype=bool) # 2D array for tunneling steps
|
| 97 |
+
|
| 98 |
+
# Create an array of masses for each quark
|
| 99 |
+
particle_masses = np.array([mass * GeV_to_J for mass in quark_masses.values()])
|
| 100 |
+
|
| 101 |
+
for j, (quark, mass) in enumerate(quark_masses.items()):
|
| 102 |
+
particle_masses_evolution[j, 0] = particle_masses[j] # Initialize mass
|
| 103 |
+
particle_speeds[j, 0] = particle_speed_initial # Initialize speed
|
| 104 |
+
particle_temperatures[j, 0] = temperature_initial # Initialize temperature
|
| 105 |
+
|
| 106 |
+
for i in range(1, num_steps):
|
| 107 |
+
# Update temperature based on expansion of the universe
|
| 108 |
+
particle_temperatures[j, i] = particle_temperatures[j, i-1] * (1 - Hubble_constant_SI * t_planck)
|
| 109 |
+
|
| 110 |
+
# Update speed using TSR
|
| 111 |
+
particle_speeds[j, i] = update_speed(particle_speeds[j, i-1], particle_temperatures[j, i], particle_masses[j])
|
| 112 |
+
|
| 113 |
+
# Apply tunneling effect
|
| 114 |
+
if np.random.rand() < tunneling_probability:
|
| 115 |
+
particle_speeds[j, i] = particle_speeds[j, 0]
|
| 116 |
+
tunneling_steps[j, i] = True
|
| 117 |
+
|
| 118 |
+
# Update mass based on energy conversion
|
| 119 |
+
energy_diff = relativistic_energy(particle_speeds[j, i], particle_masses[j]) - relativistic_energy(particle_speeds[j, i - 1], particle_masses[j])
|
| 120 |
+
particle_masses_evolution[j, i] = particle_masses_evolution[j, i - 1] + energy_diff / c**2
|
| 121 |
+
|
| 122 |
+
# Check for collisions and handle them
|
| 123 |
+
collision, idx1, idx2 = check_collision(particle_speeds[:, i], collision_distance)
|
| 124 |
+
if collision:
|
| 125 |
+
handle_collision(particle_speeds[:, i], particle_masses, idx1, idx2)
|
| 126 |
+
|
| 127 |
+
# Print calculated masses at the end of the simulation
|
| 128 |
+
print(f"Calculated masses at the end of the simulation at the colision (Tunneling Probability: {tunneling_probability}):")
|
| 129 |
+
for j, quark in enumerate(quark_masses.keys()):
|
| 130 |
+
print(f"{quark}: {particle_masses_evolution[j, -1] / GeV_to_J:.4e} GeV")
|
| 131 |
+
|
| 132 |
+
# Save data to JSON file
|
| 133 |
+
data_filename = os.path.join(data_dir, f"big_bang_simulation_data_{tunneling_probability:.2f}.json")
|
| 134 |
+
data = {
|
| 135 |
+
"tunneling_probability": tunneling_probability,
|
| 136 |
+
"particle_masses_evolution": particle_masses_evolution.tolist(),
|
| 137 |
+
"particle_speeds": particle_speeds.tolist(),
|
| 138 |
+
"particle_temperatures": particle_temperatures.tolist(),
|
| 139 |
+
"tunneling_steps": tunneling_steps.tolist()
|
| 140 |
+
}
|
| 141 |
+
with open(data_filename, "w") as f:
|
| 142 |
+
json.dump(data, f)
|
sting.py
ADDED
|
@@ -0,0 +1,48 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import numpy as np
|
| 2 |
+
import matplotlib.pyplot as plt
|
| 3 |
+
|
| 4 |
+
# Constants
|
| 5 |
+
c = 299792458 # Speed of light in m/s
|
| 6 |
+
hbar = 1.0545718e-34 # Reduced Planck constant in J·s
|
| 7 |
+
alpha = 1.0 # Fine-structure constant
|
| 8 |
+
|
| 9 |
+
# Define string properties
|
| 10 |
+
string_length = 1e-35 # Length of the string in meters
|
| 11 |
+
string_tension = 1e30 # Tension of the string in N
|
| 12 |
+
|
| 13 |
+
# Define initial conditions
|
| 14 |
+
initial_position = 0.0 # Initial position of the string
|
| 15 |
+
initial_velocity = 1e6 # Initial velocity of the string
|
| 16 |
+
|
| 17 |
+
# Simulation parameters
|
| 18 |
+
time_step = 5.39e-44 * 1e3 # Time step for the simulation
|
| 19 |
+
total_time = 5.39e-44 # Total simulation time
|
| 20 |
+
|
| 21 |
+
# Initialize arrays to store position and velocity data
|
| 22 |
+
num_steps = int(total_time / time_step) + 1
|
| 23 |
+
position = np.zeros(num_steps)
|
| 24 |
+
velocity = np.zeros(num_steps)
|
| 25 |
+
|
| 26 |
+
# Set initial conditions
|
| 27 |
+
position[0] = initial_position
|
| 28 |
+
velocity[0] = initial_velocity
|
| 29 |
+
|
| 30 |
+
# Main simulation loop
|
| 31 |
+
for i in range(1, num_steps):
|
| 32 |
+
# Calculate acceleration using string equation of motion
|
| 33 |
+
acceleration = -(string_tension / hbar) * position[i - 1]
|
| 34 |
+
|
| 35 |
+
# Update velocity and position
|
| 36 |
+
velocity[i] = velocity[i - 1] + acceleration * time_step
|
| 37 |
+
position[i] = position[i - 1] + velocity[i] * time_step
|
| 38 |
+
|
| 39 |
+
# Plot the results
|
| 40 |
+
plt.figure(figsize=(10, 6))
|
| 41 |
+
plt.plot(np.arange(num_steps) * time_step, position, label="String Position")
|
| 42 |
+
plt.xlabel("Time (s)")
|
| 43 |
+
plt.ylabel("Position (m)")
|
| 44 |
+
plt.title("String Evolution in Time")
|
| 45 |
+
plt.grid(True)
|
| 46 |
+
plt.legend()
|
| 47 |
+
plt.show()
|
| 48 |
+
|
str.py
ADDED
|
@@ -0,0 +1,48 @@
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import numpy as np
|
| 2 |
+
import matplotlib.pyplot as plt
|
| 3 |
+
|
| 4 |
+
# Constants
|
| 5 |
+
c = 299792458 # Speed of light in m/s
|
| 6 |
+
hbar = 1.0545718e-34 # Reduced Planck constant in J·s
|
| 7 |
+
alpha = 1.0 # Fine-structure constant
|
| 8 |
+
|
| 9 |
+
# Define string properties
|
| 10 |
+
string_length = 1e-35 # Length of the string in meters
|
| 11 |
+
string_tension = 1e30 # Tension of the string in N
|
| 12 |
+
|
| 13 |
+
# Define initial conditions
|
| 14 |
+
initial_position = 0.0 # Initial position of the string
|
| 15 |
+
initial_velocity = 1e6 # Initial velocity of the string
|
| 16 |
+
|
| 17 |
+
# Simulation parameters
|
| 18 |
+
time_step = 5.39e-44 * 1e3 # Time step for the simulation
|
| 19 |
+
total_time = 1e-40 # Extended total simulation time
|
| 20 |
+
|
| 21 |
+
# Initialize arrays to store position and velocity data
|
| 22 |
+
num_steps = int(total_time / time_step) + 1
|
| 23 |
+
position = np.zeros(num_steps)
|
| 24 |
+
velocity = np.zeros(num_steps)
|
| 25 |
+
|
| 26 |
+
# Set initial conditions
|
| 27 |
+
position[0] = initial_position
|
| 28 |
+
velocity[0] = initial_velocity
|
| 29 |
+
|
| 30 |
+
# Main simulation loop
|
| 31 |
+
for i in range(1, num_steps):
|
| 32 |
+
# Calculate acceleration using string equation of motion
|
| 33 |
+
acceleration = -(string_tension / hbar) * position[i - 1]
|
| 34 |
+
|
| 35 |
+
# Update velocity and position
|
| 36 |
+
velocity[i] = velocity[i - 1] + acceleration * time_step
|
| 37 |
+
position[i] = position[i - 1] + velocity[i] * time_step
|
| 38 |
+
|
| 39 |
+
# Plot the results
|
| 40 |
+
plt.figure(figsize=(10, 6))
|
| 41 |
+
plt.plot(np.arange(num_steps) * time_step, position, label="String Position")
|
| 42 |
+
plt.xlabel("Time (s)")
|
| 43 |
+
plt.ylabel("Position (m)")
|
| 44 |
+
plt.title("String Evolution in Time")
|
| 45 |
+
plt.grid(True)
|
| 46 |
+
plt.legend()
|
| 47 |
+
plt.show()
|
| 48 |
+
|
test.py
ADDED
|
@@ -0,0 +1,125 @@
|
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|
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|
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|
|
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|
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|
|
|
|
|
|
|
|
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|
|
|
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|
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|
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|
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|
|
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|
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|
|
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|
|
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|
|
|
|
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|
|
|
|
|
|
|
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|
|
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|
|
|
|
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|
|
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|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
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|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
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|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| 1 |
+
import numpy as np
|
| 2 |
+
import matplotlib.pyplot as plt
|
| 3 |
+
from matplotlib.animation import FuncAnimation
|
| 4 |
+
import cupy as cp
|
| 5 |
+
from tqdm import tqdm
|
| 6 |
+
import plotly.graph_objects as go
|
| 7 |
+
import streamlit as st
|
| 8 |
+
|
| 9 |
+
x = st.slider('Select a value')
|
| 10 |
+
st.write(x, 'squared is', x * x)
|
| 11 |
+
|
| 12 |
+
# Define the twelfth root of two
|
| 13 |
+
Q = 2 ** (1/12)
|
| 14 |
+
|
| 15 |
+
# Define the wave function of the universe with variants (using CuPy)
|
| 16 |
+
def wave_function_cupy(x, t, scale=1.0, phase_shift=0.0):
|
| 17 |
+
denominator = 2 * (t**2 + 1e-10) # Add a small value to avoid division by zero
|
| 18 |
+
return scale * Q * cp.exp(-x**2 / denominator) * cp.exp(-1j * (t + phase_shift))
|
| 19 |
+
|
| 20 |
+
# Simulation parameters
|
| 21 |
+
x = np.linspace(-10, 10, 100)
|
| 22 |
+
t = np.linspace(0, 10, 100)
|
| 23 |
+
X, T = np.meshgrid(x, t)
|
| 24 |
+
|
| 25 |
+
# Convert numpy arrays to CuPy arrays
|
| 26 |
+
X_cupy = cp.asarray(X)
|
| 27 |
+
T_cupy = cp.asarray(T)
|
| 28 |
+
|
| 29 |
+
# Variants parameters
|
| 30 |
+
scales = [0.5, 1.0, 1.5] # Different scaling factors
|
| 31 |
+
phase_shifts = [0, np.pi/4, np.pi/2] # Different phase shifts
|
| 32 |
+
|
| 33 |
+
# Initialize a 3D array to store results
|
| 34 |
+
wave_functions_3d = np.zeros((len(scales), len(phase_shifts), len(x), len(t)), dtype=complex)
|
| 35 |
+
|
| 36 |
+
# Simulate with variants and store results in the 3D array
|
| 37 |
+
for i, scale in enumerate(scales):
|
| 38 |
+
for j, phase_shift in enumerate(phase_shifts):
|
| 39 |
+
wave_functions_3d[i, j, :, :] = cp.asnumpy(wave_function_cupy(X_cupy, T_cupy, scale, phase_shift))
|
| 40 |
+
|
| 41 |
+
# --- Plotly Interactive Visualization ---
|
| 42 |
+
|
| 43 |
+
# Create the figure
|
| 44 |
+
fig = go.Figure(data=[
|
| 45 |
+
go.Surface(x=x, y=t, z=np.abs(wave_functions_3d[0, 0, :, :])**2)
|
| 46 |
+
])
|
| 47 |
+
|
| 48 |
+
fig.update_layout(
|
| 49 |
+
title="Wave Function of the Universe",
|
| 50 |
+
scene=dict(
|
| 51 |
+
xaxis_title="x",
|
| 52 |
+
yaxis_title="t",
|
| 53 |
+
zaxis_title="|ψ(x,t)|^2"
|
| 54 |
+
),
|
| 55 |
+
)
|
| 56 |
+
|
| 57 |
+
# Add Scale Slider
|
| 58 |
+
fig.update_layout(
|
| 59 |
+
sliders=[
|
| 60 |
+
dict(
|
| 61 |
+
active=True,
|
| 62 |
+
currentvalue=dict(
|
| 63 |
+
prefix="Scale: ",
|
| 64 |
+
font=dict(size=12)
|
| 65 |
+
),
|
| 66 |
+
steps=[
|
| 67 |
+
dict(
|
| 68 |
+
method="update",
|
| 69 |
+
args=[
|
| 70 |
+
{"z": [np.abs(wave_functions_3d[i, 0, :, :])**2]} # Update z data
|
| 71 |
+
],
|
| 72 |
+
label=f"Scale: {scales[i]:.2f}" # Label for step values
|
| 73 |
+
) for i in range(len(scales))
|
| 74 |
+
],
|
| 75 |
+
pad=dict(t=50),
|
| 76 |
+
len=0.9, # Length of the slider
|
| 77 |
+
x=0.1, # X position of the slider
|
| 78 |
+
y=0.1, # Y position of the slider
|
| 79 |
+
),
|
| 80 |
+
dict(
|
| 81 |
+
active=True,
|
| 82 |
+
currentvalue=dict(
|
| 83 |
+
prefix="Phase Shift: ",
|
| 84 |
+
font=dict(size=12)
|
| 85 |
+
),
|
| 86 |
+
steps=[
|
| 87 |
+
dict(
|
| 88 |
+
method="update",
|
| 89 |
+
args=[
|
| 90 |
+
{"z": [np.abs(wave_functions_3d[0, j, :, :])**2]} # Update z data
|
| 91 |
+
],
|
| 92 |
+
label=f"Phase Shift: {phase_shifts[j]:.2f}" # Label for step values
|
| 93 |
+
) for j in range(len(phase_shifts))
|
| 94 |
+
],
|
| 95 |
+
pad=dict(t=50),
|
| 96 |
+
len=0.9, # Length of the slider
|
| 97 |
+
x=0.1, # X position of the slider
|
| 98 |
+
y=0.3, # Y position of the slider
|
| 99 |
+
)
|
| 100 |
+
]
|
| 101 |
+
)
|
| 102 |
+
|
| 103 |
+
fig.show()
|
| 104 |
+
|
| 105 |
+
# --- End of Plotly ---
|
| 106 |
+
|
| 107 |
+
# --- Matplotlib Animation ---
|
| 108 |
+
|
| 109 |
+
# Animation
|
| 110 |
+
fig, ax = plt.subplots()
|
| 111 |
+
im = ax.imshow(np.abs(wave_functions_3d[0, 0, :, :]) ** 2, extent=[-10, 10, 0, 10], aspect='auto', cmap='viridis')
|
| 112 |
+
ax.set_xlabel('x')
|
| 113 |
+
ax.set_ylabel('t')
|
| 114 |
+
ax.set_title('Wave Function of the Universe')
|
| 115 |
+
cbar = fig.colorbar(im, ax=ax, label='|ψ(x,t)|^2')
|
| 116 |
+
|
| 117 |
+
def update(frame):
|
| 118 |
+
i, j = divmod(frame, len(phase_shifts)) # Get the index for the 3D array
|
| 119 |
+
im.set_array(np.abs(wave_functions_3d[i, j, :, :]) ** 2) # Update with the correct frame
|
| 120 |
+
ax.set_title(f'Wave Function at Scale: {scales[i]}, Phase Shift: {phase_shifts[j]:.2f}')
|
| 121 |
+
return im,
|
| 122 |
+
|
| 123 |
+
ani = FuncAnimation(fig, update, frames=len(scales) * len(phase_shifts), blit=True)
|
| 124 |
+
ani.save('wave_function_animation.gif', writer='pillow')
|
| 125 |
+
plt.show()
|
wave_function_animation.gif
ADDED
|