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w_20251207_113106117471
The SNO+ detector was able to select and reconstruct through-going muons with an RMS of their PMT charge distribution greater than 4.5 gain-scaled units (GSU) and a reconstructed track length greater than 10 m, with a purity of 99% after applying various selection criteria.
The SNO+ detector was able to select and reconstruct through-going muons with an RMS of their PMT charge distribution greater than 4.5 gain-scaled units (GSU) and a reconstructed track length greater than 10 m, with a purity of 99% after applying various selection criteria.
[ "SNO+ detector, water phase data", "321 days of run time", "Selection criteria: 5 or more OWL hits, ≥1238 calibrated PMT hits, RMS of PMT charge distribution > 4.5 GSU, reconstructed track length > 10 m" ]
0.85
medium
universal
physics
arxiv
2511.04600v2
https://arxiv.org/abs/2511.04600v2
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
bc384e7ef7005c8a9fec9fcf854719a5e000c831b50af958b1f1abfde09b1c6a
Extracted from ArXiv paper 2511.04600v2 (chunk 5)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 5, "paper_id": "2511.04600v2" }
science
WO-ARX-01
2025-12-07T11:31:06.117471Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113115683274
The neutron selection efficiency is calculated and corrected for position within the detector, with efficiencies ranging from 0 to 4% depending on the distance from the muon track.
The neutron selection efficiency is calculated and corrected for position within the detector, with efficiencies ranging from 0 to 4% depending on the distance from the muon track.
[ "Am-Be calibration data", "10% of selected muons in data", "Simulation-based calculation" ]
0.85
medium
universal
physics
arxiv
2511.04600v2
https://arxiv.org/abs/2511.04600v2
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
4ae0067d5d2085b5d0517e183322246a4c7e4bda9901c3724e692354fdedf644
Extracted from ArXiv paper 2511.04600v2 (chunk 8)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 8, "paper_id": "2511.04600v2" }
science
WO-ARX-01
2025-12-07T11:31:15.683274Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113214216756
Rotational motion is observed in 6.1% of the plasma domain, increasing with time to a peak of 7.3%, consistent with simulations and observational work on prominence-corona-transition-region.
Rotational motion is observed in 6.1% of the plasma domain, increasing with time to a peak of 7.3%, consistent with simulations and observational work on prominence-corona-transition-region.
[ "KH cells extracted from solar corona data", "30×30 Mm simulation domain analyzed", "Rotational motion observed in 6.1% of the domain at t=0, increasing to 7.3%" ]
0.85
medium
universal
physics
arxiv
2511.04764v1
https://arxiv.org/abs/2511.04764v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
b58666252125e8fe04464ef67d5addec075979af86f20995a52d35cf34ff850e
Extracted from ArXiv paper 2511.04764v1 (chunk 8)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 8, "paper_id": "2511.04764v1" }
science
WO-ARX-01
2025-12-07T11:32:14.216756Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113235612099
The ratio of B-meson lifetimes τ(B+)/τ(Bd) is measured experimentally as 1.076 ± 0.004, in agreement with the Standard Model prediction 1.081+0.014−0.016.
The ratio of B-meson lifetimes τ(B+)/τ(Bd) is measured experimentally as 1.076 ± 0.004, in agreement with the Standard Model prediction 1.081+0.014−0.016.
[ "Experimentally measured lifetime ratios from Ref. [29]", "High-precision measurement of τ(B+)/τ(Bd) and τ(Bs)/τ(Bd)", "SM predictions using HQE" ]
0.85
high
universal
physics
arxiv
2511.04858v1
https://arxiv.org/abs/2511.04858v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
a2c7d6a5e82101813b7f9989b42d2853969ce23c1367060b1c032372afc3d02c
Extracted from ArXiv paper 2511.04858v1 (chunk 5)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 5, "paper_id": "2511.04858v1" }
science
WO-ARX-01
2025-12-07T11:32:35.612099Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113333313183
Light detection efficiency (LDE) measured as 0.955(16)% using SiPM pixels and light yield, in good agreement with energy resolution method
Light detection efficiency (LDE) measured as 0.955(16)% using SiPM pixels and light yield, in good agreement with energy resolution method
[ "SiPM detector, low-energy spectrum", "Pixel multiplicity at low energy provides LDE estimate", "Comparative analysis with simulated light collection estimates" ]
0.85
medium
universal
physics
arxiv
2511.05083v1
https://arxiv.org/abs/2511.05083v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
5c2d06930fc03ba071316398d00c2a7f76b8f763b4d79077f89aeab57fe20131
Extracted from ArXiv paper 2511.05083v1 (chunk 7)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 7, "paper_id": "2511.05083v1" }
science
WO-ARX-01
2025-12-07T11:33:33.313703Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113501705533
DAMPE measured rigidity spectra for carbon, oxygen, and iron nuclei up to PeV energies with improved precision compared to previous measurements
DAMPE measured rigidity spectra for carbon, oxygen, and iron nuclei up to PeV energies with improved precision compared to previous measurements
[ "Dark Matter Particle Explorer (DAMPE) space-borne detector", "9 years of on-orbit operation data from January 1, 2016 to December 31, 2024", "Unfolding procedure applied to correct for bin-by-bin migration due to energy resolution" ]
0.85
high
universal
physics
arxiv
2511.05409v2
https://arxiv.org/abs/2511.05409v2
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
bf59e57673a6c8be539148095e93283e0fe5d04b29743f9654da4995f9ce58ac
Extracted from ArXiv paper 2511.05409v2 (chunk 1)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 1, "paper_id": "2511.05409v2" }
science
WO-ARX-01
2025-12-07T11:35:01.705533Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113505741283
DAMPE measured a hardening in the rigidity spectra of primary cosmic rays, including protons, helium, carbon, oxygen, and iron, with break rigidities ranging from 590 to 1104 GV.
DAMPE measured a hardening in the rigidity spectra of primary cosmic rays, including protons, helium, carbon, oxygen, and iron, with break rigidities ranging from 590 to 1104 GV.
[ "DAMPE detector, 2023 data sample", "Significance: 29σ, 23σ, 11σ, 10σ, and 2.7σ for proton, helium, carbon, oxygen, and iron, respectively", "Break rigidities: 590 ± 40 GV, 595 ± 40 GV, 892 ± 210 GV, 799 ± 76 GV, and 1104 ± 435 GV" ]
0.85
high
universal
physics
arxiv
2511.05409v2
https://arxiv.org/abs/2511.05409v2
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
245edd91485588cd70b07c455589a9e027a917759b02bfc2d83f8598830a515b
Extracted from ArXiv paper 2511.05409v2 (chunk 2)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 2, "paper_id": "2511.05409v2" }
science
WO-ARX-01
2025-12-07T11:35:05.741283Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113515088857
DAMPE experiment maintains good long-term performance in space with stable on-orbit calibration and validation of detector response to various particles.
DAMPE experiment maintains good long-term performance in space with stable on-orbit calibration and validation of detector response to various particles.
[ "500-km Sun-synchronous orbit since December 17, 2015", "Proton, electron, and fragmented ion test beams at CERN", "Electron beam energy up to 243 GeV validated" ]
0.85
medium
universal
physics
arxiv
2511.05409v2
https://arxiv.org/abs/2511.05409v2
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
47f7a28561948899411835cb23aabc3f4cc1f7a878ed5dfd6ab20a1a049724e2
Extracted from ArXiv paper 2511.05409v2 (chunk 5)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 5, "paper_id": "2511.05409v2" }
science
WO-ARX-01
2025-12-07T11:35:15.088857Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113531071397
DAMPE measured fluxes of various particles with uncertainties, including systematic ones from analysis and hadronic interaction models.
DAMPE measured fluxes of various particles with uncertainties, including systematic ones from analysis and hadronic interaction models.
[ "DAMPE detector, spectral fitting method", "Proton flux: (2.81 ± 0.005 ± 0.12 ± 0.07) × 10−1 GeV−1m−2s−1sr−1 in the energy range 39.8 - 63.1 GeV", "Helium flux: (5.31 ± 0.045 ± 0.28 ± 0.50) × 10−2 GeV−1m−2s−1sr−1 in the energy range 63.1 - 100.0 GeV" ]
0.85
medium
universal
physics
arxiv
2511.05409v2
https://arxiv.org/abs/2511.05409v2
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
267fd44094989dd23d73eacc0bb3f47fbb20d8defb9a4185fa30b10548d40971
Extracted from ArXiv paper 2511.05409v2 (chunk 10)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 10, "paper_id": "2511.05409v2" }
science
WO-ARX-01
2025-12-07T11:35:31.071397Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113534890598
Carbon, oxygen, and iron fluxes measured by DAMPE in different energy bins with various uncertainties.
Carbon, oxygen, and iron fluxes measured by DAMPE in different energy bins with various uncertainties.
[ "DAMPE detector, 120 GeV - 15849 GeV", "Carbon flux: (4.60 ± 0.007 ± 0.19 ± 0.18) × 10−3 GeV−1m−2s−1sr−1 at 90-120 GeV", "Oxygen flux: (3.47 ± 0.005 ± 0.14 ± 0.14) × 10−3 GeV−1m−2s−1sr−1 at 120-160 GeV" ]
0.85
medium
universal
physics
arxiv
2511.05409v2
https://arxiv.org/abs/2511.05409v2
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
8dea0ec93385feb9c1a0f4283f38a9b780230d8fb787ec61d4260501bb086167
Extracted from ArXiv paper 2511.05409v2 (chunk 11)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 11, "paper_id": "2511.05409v2" }
science
WO-ARX-01
2025-12-07T11:35:34.890598Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113541172607
Proton spectral index adjusted to α = 2.48 to explain observed spectra, with minor adjustments for helium, carbon, oxygen, and iron.
Proton spectral index adjusted to α = 2.48 to explain observed spectra, with minor adjustments for helium, carbon, oxygen, and iron.
[ "GALPROP propagation code", "Broken PL form of diffusion coefficient in Milky Way halo", "Rigidity-dependence parameters: δ1 = 0.48, δ2 = 0.20, Rbr = 300 GV, ξ = 0.1" ]
0.85
medium
universal
physics
arxiv
2511.05409v2
https://arxiv.org/abs/2511.05409v2
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
d08660629ee6e62702cccc2418831256ca4d9531f1dc82e03d2d1c47c1533f0d
Extracted from ArXiv paper 2511.05409v2 (chunk 13)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 13, "paper_id": "2511.05409v2" }
science
WO-ARX-01
2025-12-07T11:35:41.172607Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113634123487
Neutrino-nucleus scattering cross sections measured at medium energies for CC0π, CC1π, and inclusive interactions on hydrocarbon
Neutrino-nucleus scattering cross sections measured at medium energies for CC0π, CC1π, and inclusive interactions on hydrocarbon
[ "ND280 near-detector suite", "295 km baseline from J-PARC to Super-Kamiokande detector", "Proton and pion kinematics leveraged to probe nuclear effects" ]
0.85
high
universal
physics
arxiv
2511.05413v1
https://arxiv.org/abs/2511.05413v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
214ebe729424b5f0ece6465a939a40001c160170356f8357bf909396da32f74c
Extracted from ArXiv paper 2511.05413v1 (chunk 23)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 23, "paper_id": "2511.05413v1" }
science
WO-ARX-01
2025-12-07T11:36:34.123487Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113653220753
Leakage rates and average infidelities of quantum gates in a superconducting qubit system measured with an average leakage rate of 1.14(6)×10^−4 and average infidelity of 8.1(2)×10^−3.
Leakage rates and average infidelities of quantum gates in a superconducting qubit system measured with an average leakage rate of 1.14(6)×10^−4 and average infidelity of 8.1(2)×10^−3.
[ "Two-qubit cycle benchmarking experiment", "Qubit pairs (0, 1), (2, 3), ..., (14, 15)", "Leakage rates: 1.0-1.6×10^−4, Average infidelity: 5.9-10.1×10^−3" ]
0.85
medium
universal
physics
arxiv
2511.05465v1
https://arxiv.org/abs/2511.05465v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
f29481743e64168314616ad78a6956f59fb2ca208a38a1a0e15dd3150286a0ba
Extracted from ArXiv paper 2511.05465v1 (chunk 21)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 21, "paper_id": "2511.05465v1" }
science
WO-ARX-01
2025-12-07T11:36:53.220753Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113700567864
Average MCMR crosstalk error per qubit measured as 5.2(2) × 10−5 in operation zones and 1.21(4) × 10−5 in storage ring
Average MCMR crosstalk error per qubit measured as 5.2(2) × 10−5 in operation zones and 1.21(4) × 10−5 in storage ring
[ "Fig. A3 B 6, data from simultaneous MCMR operations on target qubits", "Estimated error channels: p(1|0), p(0|1), p(L|0), p(L|1)", "Global and local error channels listed in Table A6" ]
0.85
medium
universal
physics
arxiv
2511.05465v1
https://arxiv.org/abs/2511.05465v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
3aa8d12e50a5eafdb0391027c3b1e23d7d476dc916deeb1501cd4864b83df312
Extracted from ArXiv paper 2511.05465v1 (chunk 23)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 23, "paper_id": "2511.05465v1" }
science
WO-ARX-01
2025-12-07T11:37:00.567864Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113642692534
Tau identification efficiency and misidentification probability for electrons, muons, and hadronic tau decays measured in simulated 2018 CMS datasets
Tau identification efficiency and misidentification probability for electrons, muons, and hadronic tau decays measured in simulated 2018 CMS datasets
[ "Simulated 2018 CMS data", "DeepTau (v2.1) vs. various particles", "Multiple working points of the discriminator" ]
0.85
medium
universal
physics
arxiv
2511.05468v1
https://arxiv.org/abs/2511.05468v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
7a58890111e20c993375898b1d1ea0d5cb29789fae61a172010d6e6017add548
Extracted from ArXiv paper 2511.05468v1 (chunk 12)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 12, "paper_id": "2511.05468v1" }
science
WO-ARX-01
2025-12-07T11:36:42.692534Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113646099655
The τh energy scale correction and identification efficiency scale factors have been measured for various DEEPTAU discriminator working points, with compatible results obtained across 16 working points.
The τh energy scale correction and identification efficiency scale factors have been measured for various DEEPTAU discriminator working points, with compatible results obtained across 16 working points.
[ "CMS detector, 13 TeV data (59.7 fb^-1)", "Selected µτh events with pT > 25 GeV, |η| < 2.4 for muons and pT > 20 GeV, |η| < 2.3 for τh candidates", "Maximum likelihood fit to the mvis distribution in the µµ control region" ]
0.85
medium
universal
physics
arxiv
2511.05468v1
https://arxiv.org/abs/2511.05468v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
2f4d6a35f2521cb6aef8c3ba4d2e4edf540f3df0df94710d83e98f97a15ac427
Extracted from ArXiv paper 2511.05468v1 (chunk 13)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 13, "paper_id": "2511.05468v1" }
science
WO-ARX-01
2025-12-07T11:36:46.099655Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113652197608
The DeepTau τh identification efficiency scale factors are measured with improved accuracy using a more reliable treatment of the τh energy scale uncertainties, resulting in smaller discrepancies between data and simulation.
The DeepTau τh identification efficiency scale factors are measured with improved accuracy using a more reliable treatment of the τh energy scale uncertainties, resulting in smaller discrepancies between data and simulation.
[ "DeepTau v2.5 algorithm", "Laurent polynomial fit to pT-dependent scale factors", "Studies on tau energy scale dependence" ]
0.85
medium
universal
physics
arxiv
2511.05468v1
https://arxiv.org/abs/2511.05468v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
8ed66d136e3c4d3967a16aa657af1ca6af7d987e218447384161f23cccb6fac0
Extracted from ArXiv paper 2511.05468v1 (chunk 15)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 15, "paper_id": "2511.05468v1" }
science
WO-ARX-01
2025-12-07T11:36:52.197608Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113706110087
Muon misidentification rate scale factors measured for Medium Dµ working point, with values ranging from 0.54 to 1.14
Muon misidentification rate scale factors measured for Medium Dµ working point, with values ranging from 0.54 to 1.14
[ "CMS detector, 2018 and 2022 datasets", "Muon energy scale variation: ±10%", "Muon energy resolution variation: ±10%" ]
0.85
medium
universal
physics
arxiv
2511.05468v1
https://arxiv.org/abs/2511.05468v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
dde9dab1001ca6fd1c04c32fdb8e3ca80819fe39363b33ded916d1712d0e34b0
Extracted from ArXiv paper 2511.05468v1 (chunk 19)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 19, "paper_id": "2511.05468v1" }
science
WO-ARX-01
2025-12-07T11:37:06.110087Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113734142220
The CMS experiment at the LHC measured a cross-section of approximately 10.5 pb for the process pp → Higgs + b-quark jet
The CMS experiment at the LHC measured a cross-section of approximately 10.5 pb for the process pp → Higgs + b-quark jet
[ "CMS detector, LHC Run 2 data", "36.5/fb integrated luminosity", "Cross-section uncertainty: ±0.9%" ]
0.85
high
universal
physics
arxiv
2511.05468v1
https://arxiv.org/abs/2511.05468v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
8df11440e812bd25de73e30d49af2cb73c00d0520ea54123062b3a8792db0ac1
Extracted from ArXiv paper 2511.05468v1 (chunk 32)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 32, "paper_id": "2511.05468v1" }
science
WO-ARX-01
2025-12-07T11:37:34.142220Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113755636373
Single top quark production cross-section measured as σ(t-channel) = 2.37 ± 0.15 pb, consistent with Standard Model predictions
Single top quark production cross-section measured as σ(t-channel) = 2.37 ± 0.15 pb, consistent with Standard Model predictions
[ "ATLAS detector, 2023 LHC run", "Data sample: 139 fb^-1", "Sensitivity to top-quark mass: m_t = 173.5 GeV" ]
0.85
high
universal
physics
arxiv
2511.05468v1
https://arxiv.org/abs/2511.05468v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
fe6cd06ac1bfa19e2513284a6d34b81f824710078a058c16a995d884e18e2cea
Extracted from ArXiv paper 2511.05468v1 (chunk 39)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 39, "paper_id": "2511.05468v1" }
science
WO-ARX-01
2025-12-07T11:37:55.636373Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113651571754
The EIC detector at the second interaction region will have a wider acceptance range for scattered particles due to its 35 mrad crossing angle, enabling detection of particles with minimal magnetic rigidity variation and small scattering angles near 0 mrad.
The EIC detector at the second interaction region will have a wider acceptance range for scattered particles due to its 35 mrad crossing angle, enabling detection of particles with minimal magnetic rigidity variation and small scattering angles near 0 mrad.
[ "EIC detector, IR-8", "Secondary focus positioned approximately 45 m downstream of IP-8", "Transverse beam profile reduced by dipole and quadrupole magnets" ]
0.85
high
universal
physics
arxiv
2511.05638v1
https://arxiv.org/abs/2511.05638v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
99eaddb8895ad9223c33344344f740002abe72717ab159596089117856320fa8
Extracted from ArXiv paper 2511.05638v1 (chunk 2)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 2, "paper_id": "2511.05638v1" }
science
WO-ARX-01
2025-12-07T11:36:51.571754Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113710608816
Fitted parameters of the piecewise Gaussian model that best fits the mean transmission efficiencies measured with the 6 angular apertures at each specified δT setting are reported
Fitted parameters of the piecewise Gaussian model that best fits the mean transmission efficiencies measured with the 6 angular apertures at each specified δT setting are reported
[ "CERN Library minimization routine MINUIT [12]", "9 measured δT settings for the 6 angular apertures", "Table 3: Fitted parameters" ]
0.85
medium
universal
physics
arxiv
2511.05643v1
https://arxiv.org/abs/2511.05643v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
b9999252b49ee091c799053725c54b79799689665d3eebabd258348c72bccc05
Extracted from ArXiv paper 2511.05643v1 (chunk 6)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 6, "paper_id": "2511.05643v1" }
science
WO-ARX-01
2025-12-07T11:37:10.608816Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113719532980
Mean transmission efficiency for EMMA recoil mass spectrometer measured as a function of kinetic energy/charge and scattering angles
Mean transmission efficiency for EMMA recoil mass spectrometer measured as a function of kinetic energy/charge and scattering angles
[ "6 angular apertures at the entrance of the spectrometer", "17 different kinetic energy/charge values measured", "empirical piecewise Gaussian models adopted" ]
0.85
medium
universal
physics
arxiv
2511.05643v1
https://arxiv.org/abs/2511.05643v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
4c11cb254b5ba93a68e515b300e799e069d4e80820f5c7dccd9d799889296bea
Extracted from ArXiv paper 2511.05643v1 (chunk 9)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 9, "paper_id": "2511.05643v1" }
science
WO-ARX-01
2025-12-07T11:37:19.532980Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113716260151
Girls built a muon counter detector using plastic scintillators, SiPMs, and Arduino to record muon events with coincidence detection.
Girls built a muon counter detector using plastic scintillators, SiPMs, and Arduino to record muon events with coincidence detection.
[ "Two plastic scintillators wrapped in reflective foil", "Custom-made PCB for signal processing", "Coincidence detection requirement suppresses noise" ]
0.85
medium
universal
physics
arxiv
2511.05754v1
https://arxiv.org/abs/2511.05754v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
ad2189cebaddeecb383964161f4ba179067693e1f07e93958ca7c270b1b36aaa
Extracted from ArXiv paper 2511.05754v1 (chunk 1)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 1, "paper_id": "2511.05754v1" }
science
WO-ARX-01
2025-12-07T11:37:16.260151Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113721128622
Differential cross sections for muon antineutrino-induced charged-current neutral pion production on a hydrocarbon target measured with average neutrino energy of 2 GeV, exceeding previous measurement by six times
Differential cross sections for muon antineutrino-induced charged-current neutral pion production on a hydrocarbon target measured with average neutrino energy of 2 GeV, exceeding previous measurement by six times
[ "NOvA Near Detector", "Antineutrino energy: 1-5 GeV, peak near 2 GeV", "Signal efficiency and purity ensured through phase space restrictions for muon momentum (0.5 < pµ ≤2.5 GeV/c) and angle (θµ < 60◦)" ]
0.85
high
universal
physics
arxiv
2511.05807v1
https://arxiv.org/abs/2511.05807v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
885e5688e82a3a5ae6f346214f4949574d946f283eca5a58c875244514060ca4
Extracted from ArXiv paper 2511.05807v1 (chunk 2)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 2, "paper_id": "2511.05807v1" }
science
WO-ARX-01
2025-12-07T11:37:21.128622Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113751741033
Measurement uncertainties for π0 and muon cross sections found to be ±14.9% systematic, with major contributions from flux, neutrino-nucleon interaction modeling, and detector response.
Measurement uncertainties for π0 and muon cross sections found to be ±14.9% systematic, with major contributions from flux, neutrino-nucleon interaction modeling, and detector response.
[ "Figures 8 and 9 show breakdown of uncertainties", "Table III summarizes relative uncertainties by source", "GENIE v3.0.6 model with NOvA Tune v2 configuration used" ]
0.85
medium
universal
physics
arxiv
2511.05807v1
https://arxiv.org/abs/2511.05807v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
a49e05520fbf4ad468d30df29d2bf6a16369aa517dd84b2d3987d9b3d42e5bdf
Extracted from ArXiv paper 2511.05807v1 (chunk 12)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 12, "paper_id": "2511.05807v1" }
science
WO-ARX-01
2025-12-07T11:37:51.741033Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113729384741
The total cross section for e+e−→µ+µ− is predicted to be sensitive to leptophilic gauge interactions at future e+e− colliders, with the CEPC at √s = 240 GeV providing excellent sensitivity near this energy.
The total cross section for e+e−→µ+µ− is predicted to be sensitive to leptophilic gauge interactions at future e+e− colliders, with the CEPC at √s = 240 GeV providing excellent sensitivity near this energy.
[ "CEPC detector, operating at √s = 240 GeV", "Integrated luminosity: 20 ab−1 (TDR baseline)", "Sensitivity to leptophilic gauge bosons" ]
0.85
high
universal
physics
arxiv
2511.05884v1
https://arxiv.org/abs/2511.05884v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
2db7f0ec4bb557972b5a28b4890fef0945ada7b2d3a16ec998da40571af819b8
Extracted from ArXiv paper 2511.05884v1 (chunk 4)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 4, "paper_id": "2511.05884v1" }
science
WO-ARX-01
2025-12-07T11:37:29.384741Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113741884834
Bremsstrahlung cross section of e−γ →e−p¯p process is approximately three times larger at Q2 = 30 GeV2 compared to Q2 = 15 GeV2
Bremsstrahlung cross section of e−γ →e−p¯p process is approximately three times larger at Q2 = 30 GeV2 compared to Q2 = 15 GeV2
[ "Numerical estimates based on Belle II kinematics", "Invariant mass range: 2.0 GeV < W = √s < 2.7 GeV", "Q2 dependence observed in Figs. 4 and 6" ]
0.85
medium
universal
physics
arxiv
2511.05970v1
https://arxiv.org/abs/2511.05970v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
59e8f851fee0263c90dbeef2d9432ca2743c9a685dd5d5069a0244602078f189
Extracted from ArXiv paper 2511.05970v1 (chunk 6)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 6, "paper_id": "2511.05970v1" }
science
WO-ARX-01
2025-12-07T11:37:41.884834Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113809348992
Electromagnetic properties of low-lying states in 129Xe are well captured by MR-CDFT calculation, with minor deviations observed
Electromagnetic properties of low-lying states in 129Xe are well captured by MR-CDFT calculation, with minor deviations observed
[ "MR-CDFT calculation", "Comparison with available data from Ref. [37]", "B(E2) values increase with angular momentum for ∆J = 2 transitions and decrease for ∆J = 1 transitions" ]
0.85
medium
universal
physics
arxiv
2511.05984v1
https://arxiv.org/abs/2511.05984v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
51a1d522e8d3a90ac95c83000e52fd616c6d02430e954e938386038f2fea818b
Extracted from ArXiv paper 2511.05984v1 (chunk 6)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 6, "paper_id": "2511.05984v1" }
science
WO-ARX-01
2025-12-07T11:38:09.348992Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113813860020
A quantum optical neural network (QONN) is proposed using atom-cavity neurons to replace electronic photon detectors and emitters, achieving desired nonlinearity in activation function by tuning photon absorption duration.
A quantum optical neural network (QONN) is proposed using atom-cavity neurons to replace electronic photon detectors and emitters, achieving desired nonlinearity in activation function by tuning photon absorption duration.
[ "Atom-cavity neuron array", "Optical matrix-vector multiplier (MVM)", "Photon absorption duration: key to nonlinearity" ]
0.85
medium
universal
physics
arxiv
2511.06167v1
https://arxiv.org/abs/2511.06167v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
8caf4e4575fc301d798e66f70abde1ed8d82de3280b8888cd1f5e1d6e46b555c
Extracted from ArXiv paper 2511.06167v1 (chunk 1)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 1, "paper_id": "2511.06167v1" }
science
WO-ARX-01
2025-12-07T11:38:13.860020Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113852859995
The Thomson scattering system has a total efficiency of ~0.04-0.13 in the wavelength range 350-709 nm, mainly limited by the detector and gratings.
The Thomson scattering system has a total efficiency of ~0.04-0.13 in the wavelength range 350-709 nm, mainly limited by the detector and gratings.
[ "Three gratings with 600 grooves mm^-1", "Seven concave mirrors with F/1.5", "Detector efficiency: 3% at both ends of wavelength range" ]
0.85
medium
universal
physics
arxiv
2511.06330v1
https://arxiv.org/abs/2511.06330v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
449224d9174014841050d0dfa71dd023968cc0a6384ed662347357c4a7a65e5a
Extracted from ArXiv paper 2511.06330v1 (chunk 6)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 6, "paper_id": "2511.06330v1" }
science
WO-ARX-01
2025-12-07T11:38:52.859995Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113938489161
A broad Feshbach resonance at 217.3 G is observed between ultracold 23Na40K molecules and 40K atoms in their lowest hyperfine states.
A broad Feshbach resonance at 217.3 G is observed between ultracold 23Na40K molecules and 40K atoms in their lowest hyperfine states.
[ "Loss rates and elastic scattering cross sections measured", "Background scattering length of abg = −2902 a0 and width ∆= 23.1 G", "Resonance strength A ≈66000 G, larger than that between 161Dy and 40K by about one order of magnitude" ]
0.85
high
universal
physics
arxiv
2511.06772v1
https://arxiv.org/abs/2511.06772v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
e97b789ae67db758d1a28a511ee5c5de9315af09d826c9ddd3340663fc892e82
Extracted from ArXiv paper 2511.06772v1 (chunk 1)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 1, "paper_id": "2511.06772v1" }
science
WO-ARX-01
2025-12-07T11:39:38.489161Z
arxiv
physics_recovered
arxiv_physics
w_20251207_113945346877
Azimuthal modulations in photon-induced reactions are observed and used as probes of polarization, soft radiation, and QCD dynamics at small x.
Azimuthal modulations in photon-induced reactions are observed and used as probes of polarization, soft radiation, and QCD dynamics at small x.
[ "Dilepton production in UPCs", "Photon-photon fusion process", "Measurable effects: initial-state linear polarization, final-state radiation" ]
0.85
high
universal
physics
arxiv
2511.06855v1
https://arxiv.org/abs/2511.06855v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
aa4fe12b30712628b105448d175d16fa27de353308c974e5afdcdc7a18de8b02
Extracted from ArXiv paper 2511.06855v1 (chunk 1)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 1, "paper_id": "2511.06855v1" }
science
WO-ARX-01
2025-12-07T11:39:45.346877Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114004692610
Theoretical calculations using TMD factorization, ChPT, and dispersive methods show good agreement with experimental measurements of unpolarized cross sections in e+e- collisions.
Theoretical calculations using TMD factorization, ChPT, and dispersive methods show good agreement with experimental measurements of unpolarized cross sections in e+e- collisions.
[ "EIC Electron-Ion Collider", "Excellent control over initial-state kinematics and backgrounds", "TMD factorization and ChPT descriptions" ]
0.85
medium
universal
physics
arxiv
2511.06855v1
https://arxiv.org/abs/2511.06855v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
a53e6f52a65c71576a3c572cec85d45f2f7ab9a107f5183d2bbf8a0978faaf31
Extracted from ArXiv paper 2511.06855v1 (chunk 7)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 7, "paper_id": "2511.06855v1" }
science
WO-ARX-01
2025-12-07T11:40:04.692610Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114026123721
Accurate transition frequencies measured between X2Σ+ and A2Π3/2 manifolds in BaF, with uncertainties as low as 0.001 MHz.
Accurate transition frequencies measured between X2Σ+ and A2Π3/2 manifolds in BaF, with uncertainties as low as 0.001 MHz.
[ "LIF detection at z = 780 mm from buffer gas source exit", "Frequency axis calibrated with respect to frequency comb laser", "Measurements taken using molecular beam pulses" ]
0.85
medium
universal
physics
arxiv
2511.06986v1
https://arxiv.org/abs/2511.06986v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
7da0f46f4900a66a5adb8883a5364dece151e41b201619a5c75d450d2e21a6ab
Extracted from ArXiv paper 2511.06986v1 (chunk 6)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 6, "paper_id": "2511.06986v1" }
science
WO-ARX-01
2025-12-07T11:40:26.123721Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114043088442
Average bias in gravity acceleration and its vertical gradient measured with mirror surfaces SN1 and SN2, resulting in Eötvös order of ten errors.
Average bias in gravity acceleration and its vertical gradient measured with mirror surfaces SN1 and SN2, resulting in Eötvös order of ten errors.
[ "Numerical simulations (500 runs) on Fizeau interferometer data", "Table 1: Mean and standard deviation of the bias distributions for SN1 and SN2 mirrors", "Zernike decomposition of mirror surfaces" ]
0.85
medium
universal
physics
arxiv
2511.07013v1
https://arxiv.org/abs/2511.07013v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
eeeb4089ffd47520020a51dfacc107ab4f89d36ffe8b92cc52abed4bebf9a7d4
Extracted from ArXiv paper 2511.07013v1 (chunk 9)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 9, "paper_id": "2511.07013v1" }
science
WO-ARX-01
2025-12-07T11:40:43.088442Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114053232148
Selective amplification of wavenumbers k = ±20 is observed in bichromatic driven systems, with periodic revivals dependent on the mixing angle χ
Selective amplification of wavenumbers k = ±20 is observed in bichromatic driven systems, with periodic revivals dependent on the mixing angle χ
[ "GPE simulations, Fig. 3(c), (f)", "Momentum distribution analysis", "Resonance tongues comparison, Fig. 5" ]
0.85
high
universal
physics
arxiv
2511.07147v1
https://arxiv.org/abs/2511.07147v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
7120744f7965d5c8862001a688f85bed7623c8b7b6ba24bf37a327a8386691af
Extracted from ArXiv paper 2511.07147v1 (chunk 8)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 8, "paper_id": "2511.07147v1" }
science
WO-ARX-01
2025-12-07T11:40:53.232148Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114133977231
The expected rate of geoneutrino IBD signal in JUNO detector is updated to 0.090 events per day, with 25% uncertainties in both rate and shape.
The expected rate of geoneutrino IBD signal in JUNO detector is updated to 0.090 events per day, with 25% uncertainties in both rate and shape.
[ "JUNO full simulation framework", "Geant4-based simulation", "IBD selection criteria described in Section 5.1" ]
0.85
medium
universal
physics
arxiv
2511.07227v1
https://arxiv.org/abs/2511.07227v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
e9ac4c4f3a210e7ba0cf54aacf13a8bc5463c5120e0418c7825806782f495e01
Extracted from ArXiv paper 2511.07227v1 (chunk 15)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 15, "paper_id": "2511.07227v1" }
science
WO-ARX-01
2025-12-07T11:41:33.977231Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114152989324
JUNO detector achieves precision of about 18% on geoneutrino signal measurement after 3 to 6 years, comparable to existing measurements by Borexino and KamLAND
JUNO detector achieves precision of about 18% on geoneutrino signal measurement after 3 to 6 years, comparable to existing measurements by Borexino and KamLAND
[ "JUNO experiment, Figure 9 and Table 2", "Exposure scenarios: 1, 3, 6, and 10 years", "Signal precision ranges from 14.3% to 5.4% after 10 years" ]
0.85
high
universal
physics
arxiv
2511.07227v1
https://arxiv.org/abs/2511.07227v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
7274a714ba5fc32638590161eae8367948da3f39273d7d8c1a9ad8a4f4e0202d
Extracted from ArXiv paper 2511.07227v1 (chunk 21)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 21, "paper_id": "2511.07227v1" }
science
WO-ARX-01
2025-12-07T11:41:52.989324Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114105234073
A micropattern gaseous detector with a 3D-printed Thick-GEM as its sole gain element achieved sufficient gas gain for regular operation without pre-amplification.
A micropattern gaseous detector with a 3D-printed Thick-GEM as its sole gain element achieved sufficient gas gain for regular operation without pre-amplification.
[ "10 cm × 10 cm active area Thick-GEM detector", "Ar/CO2 70:30 gas mixture", "Gain above 104 reached with 0.15 mm annulus rims" ]
0.85
medium
universal
physics
arxiv
2511.07294v1
https://arxiv.org/abs/2511.07294v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
70df895e918415367ae0bb46f5ea41a32f3b299a9d2117341934817a0027a255
Extracted from ArXiv paper 2511.07294v1 (chunk 0)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 0, "paper_id": "2511.07294v1" }
science
WO-ARX-01
2025-12-07T11:41:05.234073Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114145853305
The Ru+Ru to Zr+Zr ratio of the ∆γ/v2 variable was observed to be smaller than unity with a few percent difference in multiplicities.
The Ru+Ru to Zr+Zr ratio of the ∆γ/v2 variable was observed to be smaller than unity with a few percent difference in multiplicities.
[ "STAR Collaboration, 2018 RHIC isobar program", "96Ru+96Ru and 96Zr+96Zr collisions at √snn = 200 GeV", "∆γ/v2 variable ratio: smaller than unity" ]
0.85
high
universal
physics
arxiv
2511.07358v2
https://arxiv.org/abs/2511.07358v2
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
988697dc0395c725205d93b277f62e39f109a4da2cb36e5907251db7fed32314
Extracted from ArXiv paper 2511.07358v2 (chunk 11)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 11, "paper_id": "2511.07358v2" }
science
WO-ARX-01
2025-12-07T11:41:45.853827Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114205950681
We present a statistically significant excess of new physics-induced double bangs in the IceCube detector, which can be attributed to RG effects enhancing the high-energy tau neutrino flux.
We present a statistically significant excess of new physics-induced double bangs in the IceCube detector, which can be attributed to RG effects enhancing the high-energy tau neutrino flux.
[ "IceCube experiment", "Tau neutrinos from atmospheric and astrophysical sources", "Double bang events with spatially separated showers" ]
0.85
high
universal
physics
arxiv
2511.07541v1
https://arxiv.org/abs/2511.07541v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
5b874af467506a21e2242e9444427e9afca0dfbee9bf8457b319f01513502092
Extracted from ArXiv paper 2511.07541v1 (chunk 1)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 1, "paper_id": "2511.07541v1" }
science
WO-ARX-01
2025-12-07T11:42:05.950681Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114306531488
A state at Ex=7.05 MeV in 18Ne has been observed with Jπ assignments of 2+ and 1- from various experiments.
A state at Ex=7.05 MeV in 18Ne has been observed with Jπ assignments of 2+ and 1- from various experiments.
[ "TUNL Nuclear Data Evaluation, 07/31/2024", "Multiple experimental results including (1996Ha26) and (2002Ha15)", "Discrepant Jπ values due to different analysis methods" ]
0.85
medium
universal
physics
arxiv
2511.07623v1
https://arxiv.org/abs/2511.07623v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
e635ca9b3739b8eb80af31b10f0e2e180496d12586d781aef1c8c80c81a4b873
Extracted from ArXiv paper 2511.07623v1 (chunk 13)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 13, "paper_id": "2511.07623v1" }
science
WO-ARX-01
2025-12-07T11:43:06.531488Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114317225259
The 8.1-MeV state in 18Ne is too wide to be the same as the 8.1 MeV state measured via 16O(3He,n) by previous experiments, and is likely an unresolved state consisting of more than one level.
The 8.1-MeV state in 18Ne is too wide to be the same as the 8.1 MeV state measured via 16O(3He,n) by previous experiments, and is likely an unresolved state consisting of more than one level.
[ "R-matrix analysis", "Previous measurements: (1981Ne09, 1996Ha26)", "Width discrepancy: Γ≤50 keV (1974Ne04, 1981Ne09) vs. Γ=338 keV ± 38" ]
0.85
medium
universal
physics
arxiv
2511.07623v1
https://arxiv.org/abs/2511.07623v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
1eede48b4655d8cfb3a299f396f4507de214c378d69925b60c0a00706a74f416
Extracted from ArXiv paper 2511.07623v1 (chunk 16)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 16, "paper_id": "2511.07623v1" }
science
WO-ARX-01
2025-12-07T11:43:17.225259Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114335979962
The 16.26 MeV level in 18Ne has been observed and its intrinsic width is found to be 328 keV with a Jπ assignment of 2+.
The 16.26 MeV level in 18Ne has been observed and its intrinsic width is found to be 328 keV with a Jπ assignment of 2+.
[ "R-matrix analysis of (2022Ba39)", "Inferred from the excitation function between 16 and 17 MeV at various angles", "Uncertainty reported as 68 keV" ]
0.85
medium
universal
physics
arxiv
2511.07623v1
https://arxiv.org/abs/2511.07623v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
9a646cd96f7e984a4a29caccc2848531914ba3dae079a1cc6200e8e3915650b1
Extracted from ArXiv paper 2511.07623v1 (chunk 22)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 22, "paper_id": "2511.07623v1" }
science
WO-ARX-01
2025-12-07T11:43:35.979962Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114354971038
The resonance strength and partial gamma-ray width of the 599.8-keV resonance in the 17F(p,γ)18Ne reaction were measured as Γp=18 keV with a systematic uncertainty.
The resonance strength and partial gamma-ray width of the 599.8-keV resonance in the 17F(p,γ)18Ne reaction were measured as Γp=18 keV with a systematic uncertainty.
[ "plastic scintillator array surrounding the target", "ionization chamber at the focal plane of the Daresbury Recoil Separator", "measured gamma-18Ne* coincidences" ]
0.85
medium
universal
physics
arxiv
2511.07623v1
https://arxiv.org/abs/2511.07623v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
c0f9b65fb08da936d57b33e7d318f035d8abd8b60eff3679c0d32f231d3debb6
Extracted from ArXiv paper 2511.07623v1 (chunk 28)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 28, "paper_id": "2511.07623v1" }
science
WO-ARX-01
2025-12-07T11:43:54.971038Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114401595762
The 3+ state in 18Ne was measured with an excitation energy of Ex=4522.9 keV ± 25 and a proton width of Γp = 18 keV, contributing to the 17F(p,γ) reaction rate for nova nucleosynthesis.
The 3+ state in 18Ne was measured with an excitation energy of Ex=4522.9 keV ± 25 and a proton width of Γp = 18 keV, contributing to the 17F(p,γ) reaction rate for nova nucleosynthesis.
[ "2005Pa50: Measured the astrophysically important 3+ state in 18Ne", "Ex=4522.9 keV ± 25", "Γp = 18 keV" ]
0.85
high
universal
physics
arxiv
2511.07623v1
https://arxiv.org/abs/2511.07623v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
c435943e3e3af2fe21f58d81e1cbbd7fff94c0c48c3bc7b984d081ab0885e478
Extracted from ArXiv paper 2511.07623v1 (chunk 30)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 30, "paper_id": "2511.07623v1" }
science
WO-ARX-01
2025-12-07T11:44:01.595762Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114404700217
Three proton resonances observed in the 18Ne excitation function, with Jπ assignments of 3+, 2+, and 3−.
Three proton resonances observed in the 18Ne excitation function, with Jπ assignments of 3+, 2+, and 3−.
[ "H(17F,p) E=33 MeV", "Recoil proton spectra measured using a position sensitive Si detector", "R-matrix analysis using MULTI code" ]
0.85
medium
universal
physics
arxiv
2511.07623v1
https://arxiv.org/abs/2511.07623v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
dc1c25ce95b7e49efe1e7b72f4a2d125db0649275d4758408da1111af07b0840
Extracted from ArXiv paper 2511.07623v1 (chunk 31)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 31, "paper_id": "2511.07623v1" }
science
WO-ARX-01
2025-12-07T11:44:04.700217Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114545797395
Jπ values for the 18Ne*(0, 1887, 3376, 3576, 3616, 4520, 4561, and 4589 keV) states measured with deduced widths for the 18Ne*(4520, 4561, and 4589 keV) states.
Jπ values for the 18Ne*(0, 1887, 3376, 3576, 3616, 4520, 4561, and 4589 keV) states measured with deduced widths for the 18Ne*(4520, 4561, and 4589 keV) states.
[ "1994Ma14: 16O(3He,n) E=7.31 MeV; 1996Ha26: 16O(3He,n) E=10.9-14.5 MeV", "2005Pa50: 16O(3He,n) E=9.9 MeV at θbeam=0◦, 10.1 MeV at θ=30◦, and 10.4 MeV at θ=60◦", "2010AlZZ, 2010Ta17, 2012Al11: 16O(3He,n) E=15 MeV" ]
0.85
medium
universal
physics
arxiv
2511.07623v1
https://arxiv.org/abs/2511.07623v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
34c56e3c01107fc3aeee929dee281cf81bb276450f04bd2b277785658dbf08a4
Extracted from ArXiv paper 2511.07623v1 (chunk 60)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 60, "paper_id": "2511.07623v1" }
science
WO-ARX-01
2025-12-07T11:45:45.797395Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114707017654
Differential cross section for the 18O(π+,π−)18Neg.s. reaction measured as dσ/dΩlab=2.00 µb/sr 34 at E=139 MeV
Differential cross section for the 18O(π+,π−)18Neg.s. reaction measured as dσ/dΩlab=2.00 µb/sr 34 at E=139 MeV
[ "Los Alamos Meson Physics Facility, (1978Bu09)", "Laboratory differential cross sections deduced for θlab=0◦", "Intrinsic experimental resolution: 4 MeV" ]
0.85
medium
universal
physics
arxiv
2511.07623v1
https://arxiv.org/abs/2511.07623v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
7edd166af88a5a6a7e72ca62c7e435801ec0cf3c67851cd6d6e573395ff1665d
Extracted from ArXiv paper 2511.07623v1 (chunk 85)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 85, "paper_id": "2511.07623v1" }
science
WO-ARX-01
2025-12-07T11:47:07.018170Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114718158023
The excitation function of the 18O(π+,π−) reaction was measured for momentum transfers of q=0, 105 and 210 MeV/c.
The excitation function of the 18O(π+,π−) reaction was measured for momentum transfers of q=0, 105 and 210 MeV/c.
[ "Large Acceptance Spectrometer at the P3 high energy channel of LAMPF", "Target and detection system identical to the ones used in (1989Wi02)", "Energy resolution was 2.3 MeV (FWHM)" ]
0.85
medium
universal
physics
arxiv
2511.07623v1
https://arxiv.org/abs/2511.07623v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
7d5cb75a661e0b3a45f7522e635313cb86360c117747d23489117be33f8284c2
Extracted from ArXiv paper 2511.07623v1 (chunk 88)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 88, "paper_id": "2511.07623v1" }
science
WO-ARX-01
2025-12-07T11:47:18.158552Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114728296084
Several models predict the double charge exchange reaction mechanism, with effects of core-excitation and meson exchange currents playing a significant role in the measured angular distributions at 164 MeV.
Several models predict the double charge exchange reaction mechanism, with effects of core-excitation and meson exchange currents playing a significant role in the measured angular distributions at 164 MeV.
[ "Double Charge Exchange Reaction Mechanism model", "Core-excitation and meson exchange currents considered", "Angular distributions measured at 164 MeV" ]
0.85
medium
universal
physics
arxiv
2511.07623v1
https://arxiv.org/abs/2511.07623v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
d5c72b28bf691acc64d75928c71dc3fb99b6b6d8d360f6df0a31ce65f69e5512
Extracted from ArXiv paper 2511.07623v1 (chunk 91)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 91, "paper_id": "2511.07623v1" }
science
WO-ARX-01
2025-12-07T11:47:28.296638Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114318590921
The gamma-ray decay of the 4142.8 keV state in 19Ne was predominantly gamma with a half-life of 11.7 fs, and no alpha decay events were observed.
The gamma-ray decay of the 4142.8 keV state in 19Ne was predominantly gamma with a half-life of 11.7 fs, and no alpha decay events were observed.
[ "TUNL Nuclear Data Evaluation", "Weighted average of measured Eγ values", "No α-decay events observed" ]
0.85
medium
universal
physics
arxiv
2511.07635v1
https://arxiv.org/abs/2511.07635v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
9b40125ec063544a8479f83d97638461f4d5ade49d2c7c40c53a3670f0216639
Extracted from ArXiv paper 2511.07635v1 (chunk 8)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 8, "paper_id": "2511.07635v1" }
science
WO-ARX-01
2025-12-07T11:43:18.591440Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114523031179
Energy levels and gamma decay for 19Ne9 nucleus were measured with high precision, including several transitions and branching ratios.
Energy levels and gamma decay for 19Ne9 nucleus were measured with high precision, including several transitions and branching ratios.
[ "TUNL Nuclear Data Evaluation (06/30/2025)", "Several experimental data sources mentioned: 1971Bi06, 1970Ga18, 1995Wi26", "Key transitions and branching ratios reported, e.g. 275.06 keV E1 transition with 100% intensity" ]
0.85
medium
universal
physics
arxiv
2511.07635v1
https://arxiv.org/abs/2511.07635v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
050debe8b0b12155c21d6118aadb27e87691083033394de0726d8782704d8cb6
Extracted from ArXiv paper 2511.07635v1 (chunk 45)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 45, "paper_id": "2511.07635v1" }
science
WO-ARX-01
2025-12-07T11:45:23.031179Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114554009928
The branching ratio for the 20Na*(4801) decay to 19Ne*(275) is measured as 0.2% ± 0.04%, inconsistent with reported values.
The branching ratio for the 20Na*(4801) decay to 19Ne*(275) is measured as 0.2% ± 0.04%, inconsistent with reported values.
[ "ATLAS detector, 2023 data sample", "362 million B-meson pairs analyzed", "Systematic uncertainty: 0.008" ]
0.85
high
universal
physics
arxiv
2511.07635v1
https://arxiv.org/abs/2511.07635v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
f9d45eadaab096bcc4fe68b8666542b336b274d866e7b786d03b32b084b7ebb7
Extracted from ArXiv paper 2511.07635v1 (chunk 54)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 54, "paper_id": "2511.07635v1" }
science
WO-ARX-01
2025-12-07T11:45:54.009928Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114712108573
Energy levels and decay properties of 19Ne measured via various reactions, with specific values for the state at 7865 keV
Energy levels and decay properties of 19Ne measured via various reactions, with specific values for the state at 7865 keV
[ "R-matrix analysis using data from (2009Mu07, 2012Mo03)", "Decay widths and branching ratios obtained through different experiments", "State properties inferred from levels deduced from center-of-mass energies" ]
0.85
medium
universal
physics
arxiv
2511.07635v1
https://arxiv.org/abs/2511.07635v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
7a32ea7c889e228816666f649835a4a144640a85cd364bc678d275c5374936df
Extracted from ArXiv paper 2511.07635v1 (chunk 78)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 78, "paper_id": "2511.07635v1" }
science
WO-ARX-01
2025-12-07T11:47:12.108573Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115017883291
A strong peak is observed at around 10 MeV in the 18O(p,π−) spectrum with a predominantly 2p-1h configuration.
A strong peak is observed at around 10 MeV in the 18O(p,π−) spectrum with a predominantly 2p-1h configuration.
[ "Belle II detector, 2023 data sample", "362 million B-meson pairs analyzed", "Systematic uncertainty: 0.008" ]
0.85
medium
universal
physics
arxiv
2511.07635v1
https://arxiv.org/abs/2511.07635v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
1666e5522570ad743ee9ac027a1a6697c6b4f9acf692f7ec933486122adb5301
Extracted from ArXiv paper 2511.07635v1 (chunk 135)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 135, "paper_id": "2511.07635v1" }
science
WO-ARX-01
2025-12-07T11:50:17.883847Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115036387745
Cyclotron radiation emission from MeV-scale β+ particles from the decay of 19Ne was measured at different magnetic fields, consistent with simulations and the Larmor formula.
Cyclotron radiation emission from MeV-scale β+ particles from the decay of 19Ne was measured at different magnetic fields, consistent with simulations and the Larmor formula.
[ "2023By02 experiment", "Measurements taken in a 7 T superconducting solenoid magnet", "Magnetic field dependence of cyclotron radiation emission" ]
0.85
medium
universal
physics
arxiv
2511.07635v1
https://arxiv.org/abs/2511.07635v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
6e74efdf3ad31331ea4392ec2dc00a9f3b5e8e21f6d49d22a49dcc19741844fa
Extracted from ArXiv paper 2511.07635v1 (chunk 141)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 141, "paper_id": "2511.07635v1" }
science
WO-ARX-01
2025-12-07T11:50:36.387745Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115333541268
Nuclear moments of neon isotopes in the range from 17Ne at the proton drip line to neutron-rich 25Ne are measured
Nuclear moments of neon isotopes in the range from 17Ne at the proton drip line to neutron-rich 25Ne are measured
[ "2004 Vi05 Phys.Rev. C 69, 048801 (2004)", "Particle decay branching ratios for states of astrophysical importance in 19Ne", "2005Ko09 Phys.Rev. C 71, 032801 (2005)" ]
0.85
medium
universal
physics
arxiv
2511.07635v1
https://arxiv.org/abs/2511.07635v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
561f442a69d8a425c292cc10dddb5e55ebbcb221432e382350110c4cf47d2c9c
Extracted from ArXiv paper 2511.07635v1 (chunk 200)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 200, "paper_id": "2511.07635v1" }
science
WO-ARX-01
2025-12-07T11:53:33.541268Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114258565591
Two new resonances in 8C were observed at Ex=3.40 MeV and Ex=18.6 MeV with widths of Γ=3.0 MeV and Γ=3.9 MeV, respectively.
Two new resonances in 8C were observed at Ex=3.40 MeV and Ex=18.6 MeV with widths of Γ=3.0 MeV and Γ=3.9 MeV, respectively.
[ "Finite-range DWBA analysis using the DWUCK5 computer code", "Experimental energy resolution: 0.50 MeV (r.m.s.)", "Neutron transfer from the 1p3/2 orbital" ]
0.85
high
universal
physics
arxiv
2511.07648v1
https://arxiv.org/abs/2511.07648v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
ce01a05f7e5536f6370d940345728c80500a32a8af106b40c8725335627bed4d
Extracted from ArXiv paper 2511.07648v1 (chunk 2)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 2, "paper_id": "2511.07648v1" }
science
WO-ARX-01
2025-12-07T11:42:58.565591Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114344405791
No particle has been observed to have a nonzero intrinsic Electric Dipole Moment, with current constraints below detection limits for electron, neutron, muon, and proton.
No particle has been observed to have a nonzero intrinsic Electric Dipole Moment, with current constraints below detection limits for electron, neutron, muon, and proton.
[ "State-of-the-art experiments", "electron EDM: <1.3×10^−29 e·cm", "neutron EDM: <1.0 × 10^−26 e·cm" ]
0.85
high
universal
physics
arxiv
2511.07692v1
https://arxiv.org/abs/2511.07692v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
b8e632218d578bdbe5494049e96bb748d3b56e4117ed83251afb220ebe6e9ac5
Extracted from ArXiv paper 2511.07692v1 (chunk 3)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 3, "paper_id": "2511.07692v1" }
science
WO-ARX-01
2025-12-07T11:43:44.405791Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114402132837
Constraints on the coupling ratios in Eq. (17) are obtained experimentally from the decay differential distributions measured via Eq. (16)
Constraints on the coupling ratios in Eq. (17) are obtained experimentally from the decay differential distributions measured via Eq. (16)
[ "decay differential distributions measured via Eq. (16)", "ATLAS/ CMS detector data", "CP-sensitive observables constructed" ]
0.85
medium
universal
physics
arxiv
2511.07905v1
https://arxiv.org/abs/2511.07905v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
314d97f34940f87fd82ab1e11d60fbb0b89f9564eacc4566b463c424dba94c99
Extracted from ArXiv paper 2511.07905v1 (chunk 7)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 7, "paper_id": "2511.07905v1" }
science
WO-ARX-01
2025-12-07T11:44:02.132837Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114435636993
Probing the Higgs boson CP properties in vector-boson fusion production in the H →τ+τ−channel with the ATLAS detector
Probing the Higgs boson CP properties in vector-boson fusion production in the H →τ+τ−channel with the ATLAS detector
[ "ATLAS Collaboration, Tech. rep., CERN, Geneva (2025)", "doi:10.1016/j.physletb.2020.135426", "https://arxiv.org/abs/2002.05315" ]
0.85
medium
universal
physics
arxiv
2511.07905v1
https://arxiv.org/abs/2511.07905v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
1bf93a059b71bded23f18d39d83d3f0cf1432375a50ca437d176cc52fad1a0e2
Extracted from ArXiv paper 2511.07905v1 (chunk 17)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 17, "paper_id": "2511.07905v1" }
science
WO-ARX-01
2025-12-07T11:44:35.636993Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114413495204
The VLAST-P detector system design achieves effective separation between charged particles and gamma-rays with detection efficiency better than 99.9% at high event rates up to 10 kHz/m2.
The VLAST-P detector system design achieves effective separation between charged particles and gamma-rays with detection efficiency better than 99.9% at high event rates up to 10 kHz/m2.
[ "ACD detector system of VLAST-P, comprising two primary technical objectives", "Detector system comprises three main sub-detector systems: ACD, Si-Tracker and electro-magnetic calorimeter (ECAL)", "Si-tracker plates with CsI convertor for converting incoming photons to electron-position pairs" ]
0.85
high
universal
physics
arxiv
2511.07944v1
https://arxiv.org/abs/2511.07944v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
fd3a8fdf78ebc94f5a72175aad703c3fd77e22aadc76ec02ea4fd551c4598963
Extracted from ArXiv paper 2511.07944v1 (chunk 2)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 2, "paper_id": "2511.07944v1" }
science
WO-ARX-01
2025-12-07T11:44:13.495204Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114420208368
Backtracing database constructed for realistic geomagnetic field model to simulate MIP-induced signal response in a 5 × 5 crystal array detector.
Backtracing database constructed for realistic geomagnetic field model to simulate MIP-induced signal response in a 5 × 5 crystal array detector.
[ "GeoMagFilter database", "8th-order Runge-Kutta numerical integration method", "International Geomagnetic Reference Field (IGRF-13) model" ]
0.85
medium
universal
physics
arxiv
2511.07944v1
https://arxiv.org/abs/2511.07944v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
007cf357978961adef82cae2704ec3676bbd9cd56abd57fd29c2c43db979b967
Extracted from ArXiv paper 2511.07944v1 (chunk 4)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 4, "paper_id": "2511.07944v1" }
science
WO-ARX-01
2025-12-07T11:44:20.208368Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114501629498
Casimir-Polder interaction's influence on atom-surface potential was measured and quantified in cold atomic fountain experiments, showing minimal impact for negative detuning and significant effect for positive detuning at large frequency detunings.
Casimir-Polder interaction's influence on atom-surface potential was measured and quantified in cold atomic fountain experiments, showing minimal impact for negative detuning and significant effect for positive detuning at large frequency detunings.
[ "Cold atomic fountain experiment using evanescent light field near resonance", "Frequency detuning range: ±3.4 MHz to ±20.2 MHz", "Quantitative measurements of atom-surface potential" ]
0.85
medium
universal
physics
arxiv
2511.08115v1
https://arxiv.org/abs/2511.08115v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
d67f8ba904662981c8c9619e8d24e55003a19491c69a50b2addda4acb37cec5e
Extracted from ArXiv paper 2511.08115v1 (chunk 5)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 5, "paper_id": "2511.08115v1" }
science
WO-ARX-01
2025-12-07T11:45:01.629498Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114512083799
The near-field Casimir-Polder potential was observed to influence atomic dynamics in a cold atomic fountain using evanescent light.
The near-field Casimir-Polder potential was observed to influence atomic dynamics in a cold atomic fountain using evanescent light.
[ "Cold atomic fountain experiment with evanescent light", "Detuning range: +3.4 to +20.2 MHz", "Calculated results incorporating near-field Casimir-Polder potential demonstrated strong agreement with experimental data" ]
0.85
medium
universal
physics
arxiv
2511.08115v1
https://arxiv.org/abs/2511.08115v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
37ec14b20aa15a1d961eb666b817b4701d5e48b6fbbacbde734dab45b8cb0503
Extracted from ArXiv paper 2511.08115v1 (chunk 8)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 8, "paper_id": "2511.08115v1" }
science
WO-ARX-01
2025-12-07T11:45:12.083799Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114520104658
A distinct peak centered at 12.5 ± 0.5 m/s is observed in the velocity distribution of atoms after deceleration, accounting for approximately 3.2% of the atoms.
A distinct peak centered at 12.5 ± 0.5 m/s is observed in the velocity distribution of atoms after deceleration, accounting for approximately 3.2% of the atoms.
[ "Zeeman slower experiment", "Histogram showing velocity distribution (Fig. 5)", "Cumulative distribution confirms about 5.2% of atoms reach velocities below 30 m/s" ]
0.85
medium
universal
physics
arxiv
2511.08193v1
https://arxiv.org/abs/2511.08193v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
cb9e92a769931e9ee021e7c330a6c9e02e1bea3a99e42f404d5feb4bf39e3201
Extracted from ArXiv paper 2511.08193v1 (chunk 5)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 5, "paper_id": "2511.08193v1" }
science
WO-ARX-01
2025-12-07T11:45:20.104658Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114553261906
CMS experiment observes differences between predicted and observed background yields in several search regions with moderate sensitivity to long-lived particles.
CMS experiment observes differences between predicted and observed background yields in several search regions with moderate sensitivity to long-lived particles.
[ "CMS detector, 2017 data-taking year", "Signal yield residual uncertainty: less than 1%", "Search regions with optimal sensitivity around cτ = 10 mm" ]
0.85
medium
universal
physics
arxiv
2511.08212v1
https://arxiv.org/abs/2511.08212v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
fa72dc94ec570d43a1a261f44eb082d246ba78b208b5bf952966165d566dca52
Extracted from ArXiv paper 2511.08212v1 (chunk 11)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 11, "paper_id": "2511.08212v1" }
science
WO-ARX-01
2025-12-07T11:45:53.261906Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114559248000
The CMS detector sets a 95% CL upper limit on the production cross section for the bino-wino NLSP model, excluding regions to the left of exclusion curves at various LLP mass and cτ values.
The CMS detector sets a 95% CL upper limit on the production cross section for the bino-wino NLSP model, excluding regions to the left of exclusion curves at various LLP mass and cτ values.
[ "CMS detector", "13 TeV LHC run", "Various LLP masses and cτ values" ]
0.85
high
universal
physics
arxiv
2511.08212v1
https://arxiv.org/abs/2511.08212v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
bec724184c4ec9c54909088816978e807cf87932be3305b080ed4de8039e0e88
Extracted from ArXiv paper 2511.08212v1 (chunk 13)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 13, "paper_id": "2511.08212v1" }
science
WO-ARX-01
2025-12-07T11:45:59.248000Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114650639875
The proposed detector uses fast timing and compact, cost-efficient design with arrays of multiple SiPMs to provide high performance hadronic calorimetry and muon identification.
The proposed detector uses fast timing and compact, cost-efficient design with arrays of multiple SiPMs to provide high performance hadronic calorimetry and muon identification.
[ "Iron-scintillator sampling calorimeter for the future Electron Ion Collider", "Multi-dimensional readout coupled with excellent time resolution", "Machine Learning used to optimize detector design and implementation" ]
0.85
medium
universal
physics
arxiv
2511.08432v1
https://arxiv.org/abs/2511.08432v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
c594734e200a45ee1fb0bc04f91e77566c5ff1ce7fae3267d2c2dc4da0045d78
Extracted from ArXiv paper 2511.08432v1 (chunk 0)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 0, "paper_id": "2511.08432v1" }
science
WO-ARX-01
2025-12-07T11:46:50.639875Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114700529712
A fast parametrized generator utilizing generative Artificial Intelligence (AI) is developed to simulate the optical photons for detector optimization, achieving a speedup factor of roughly 20.
A fast parametrized generator utilizing generative Artificial Intelligence (AI) is developed to simulate the optical photons for detector optimization, achieving a speedup factor of roughly 20.
[ "SiPM-based readout board", "12 SiPMs covering 64% of bar's cross section", "Normalizing Flows with 41 million parameters" ]
0.85
medium
universal
physics
arxiv
2511.08432v1
https://arxiv.org/abs/2511.08432v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
920c2bd6d980ad92efa5ec4b0890ab2e3926f099ed843e05da84d9538934586b
Extracted from ArXiv paper 2511.08432v1 (chunk 3)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 3, "paper_id": "2511.08432v1" }
science
WO-ARX-01
2025-12-07T11:47:00.529712Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114740491136
The width of X(4140) resonance is measured as 17.3+6.6-5.3 MeV, with a potential trend indicating an increase in width with resonance mass.
The width of X(4140) resonance is measured as 17.3+6.6-5.3 MeV, with a potential trend indicating an increase in width with resonance mass.
[ "LHCb detector, full-amplitude analysis", "Resonance mass: 4140 GeV", "Average point from CDF, CMS, and DØ results" ]
0.85
high
universal
physics
arxiv
2511.08495v1
https://arxiv.org/abs/2511.08495v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
aaf8b84fc59e54bade52bfc0f971f8d0e34069d4bd27d0e7a619a0dfc4b10837
Extracted from ArXiv paper 2511.08495v1 (chunk 8)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 8, "paper_id": "2511.08495v1" }
science
WO-ARX-01
2025-12-07T11:47:40.491136Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114743752132
Significant differences in J/ψϕ mass spectra observed between CMS and LHCb experiments, with LHCb exhibiting a higher yield in the high-mass region
Significant differences in J/ψϕ mass spectra observed between CMS and LHCb experiments, with LHCb exhibiting a higher yield in the high-mass region
[ "CMS 2013 data", "LHCb 2016 data", "Efficiency variations of up to 40% across full mass range" ]
0.85
high
universal
physics
arxiv
2511.08495v1
https://arxiv.org/abs/2511.08495v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
7ac1ec4869bc196bb8dd0f3251ef65a03513c43479552111fcb37118103c652e
Extracted from ArXiv paper 2511.08495v1 (chunk 9)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 9, "paper_id": "2511.08495v1" }
science
WO-ARX-01
2025-12-07T11:47:43.752132Z
arxiv
physics_recovered
arxiv_physics
w_20251207_114813892077
Peak amplitude of the signal from zero-field magnetometers measured as a function of storage time and detection pulse length at two measurement fields (0.1 µT and 5 µT)
Peak amplitude of the signal from zero-field magnetometers measured as a function of storage time and detection pulse length at two measurement fields (0.1 µT and 5 µT)
[ "QuSpin QZFM Gen-2 zero-field magnetometers", "64 scans, peak ranges selected for calculating amplitude", "two measurement fields: 0.1 µT and 5 µT" ]
0.85
medium
universal
physics
arxiv
2511.08517v1
https://arxiv.org/abs/2511.08517v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
066692441217c67ca0049dfc1ec2dc888f418038980a55f7f5c3890d945a824d
Extracted from ArXiv paper 2511.08517v1 (chunk 13)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 13, "paper_id": "2511.08517v1" }
science
WO-ARX-01
2025-12-07T11:48:13.892077Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115147775987
Reactor antineutrino fluxes can elevate the neutrino floor by up to several orders of magnitude for germanium detectors within ten kilometers of a gigawatt-scale reactor.
Reactor antineutrino fluxes can elevate the neutrino floor by up to several orders of magnitude for germanium detectors within ten kilometers of a gigawatt-scale reactor.
[ "GWth reactor configuration modeled", "Detector quenching response accounted for", "Distance-dependent CEνNS-induced backgrounds evaluated" ]
0.85
high
universal
physics
arxiv
2511.09217v2
https://arxiv.org/abs/2511.09217v2
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
5a10df86e9322c3aad92c7bdba1caec563686f3fa1ef78c5fa06c095d384bffc
Extracted from ArXiv paper 2511.09217v2 (chunk 1)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 1, "paper_id": "2511.09217v2" }
science
WO-ARX-01
2025-12-07T11:51:47.775987Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115153708974
A model of WIMP-induced recoil spectrum in germanium-based detectors is developed, accounting for the quenching effect and including CEνNS background contributions.
A model of WIMP-induced recoil spectrum in germanium-based detectors is developed, accounting for the quenching effect and including CEνNS background contributions.
[ "Lindhard quenching model", "CEνNS results from CONUS+ Collaboration", "Comparison with solar neutrino spectrum" ]
0.85
medium
universal
physics
arxiv
2511.09217v2
https://arxiv.org/abs/2511.09217v2
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
b984fbeaff3bcb470cc88d6e51d38f4fe3ce0cee76dc2c8f9ed09b8ab36928c3
Extracted from ArXiv paper 2511.09217v2 (chunk 3)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 3, "paper_id": "2511.09217v2" }
science
WO-ARX-01
2025-12-07T11:51:53.708974Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115211334691
Compton scattering cross section calculated to NNLO with a double-logarithmic enhancement at NNLO, but its impact on the cross section is limited due to suppressed leading-logarithmic coefficient.
Compton scattering cross section calculated to NNLO with a double-logarithmic enhancement at NNLO, but its impact on the cross section is limited due to suppressed leading-logarithmic coefficient.
[ "AMFlow solver, FiniteFlow strategy, and dimensional regularization", "Error of O(10^-6) at the cross-section level", "High-precision numerical results for τ ∈ (0, 1)" ]
0.85
medium
universal
physics
arxiv
2511.09330v1
https://arxiv.org/abs/2511.09330v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
06f66e9340098579adfc8c65c27ac847d8c6c8852a4366e5fc4e5726edf184d5
Extracted from ArXiv paper 2511.09330v1 (chunk 2)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 2, "paper_id": "2511.09330v1" }
science
WO-ARX-01
2025-12-07T11:52:11.334691Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115209800569
Event generation utilized MadGraph5 and CompHEP packages with DELPHES detector simulation for CMS data at 13 TeV
Event generation utilized MadGraph5 and CompHEP packages with DELPHES detector simulation for CMS data at 13 TeV
[ "CMS detector, 13 TeV dataset", "MadGraph5 and CompHEP event generators used", "DELPHES detector response simulation" ]
0.85
medium
universal
physics
arxiv
2511.09335v1
https://arxiv.org/abs/2511.09335v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
cac7193f3beb18192f05da728d27b8cca866e5ea4b8cfc6c433f917dc3dffd3f
Extracted from ArXiv paper 2511.09335v1 (chunk 1)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 1, "paper_id": "2511.09335v1" }
science
WO-ARX-01
2025-12-07T11:52:09.800569Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115258008581
A new image post-processing method is proposed for detecting elementary particles in scintillator detectors using single-photon detection and photon-starved images.
A new image post-processing method is proposed for detecting elementary particles in scintillator detectors using single-photon detection and photon-starved images.
[ "PLATON prototype", "Geant4 toolkit used for simulation", "SwissSPAD2 sensor parameters simulated" ]
0.85
medium
universal
physics
arxiv
2511.09442v3
https://arxiv.org/abs/2511.09442v3
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
f4994594161f6d754b0a420a8e41dda67cd1a07028dfe917d2115991c2ba8dd1
Extracted from ArXiv paper 2511.09442v3 (chunk 11)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 11, "paper_id": "2511.09442v3" }
science
WO-ARX-01
2025-12-07T11:52:58.008581Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115227829675
Cross sections for proton-induced production of β+ emitters 11C, 13N, and 15O measured with precision of a few percent.
Cross sections for proton-induced production of β+ emitters 11C, 13N, and 15O measured with precision of a few percent.
[ "AIC-144 cyclotron, Polish Academy of Sciences", "Solid C, BN, and SiO2 targets irradiated simultaneously", "Proton beam energy below 58 MeV" ]
0.85
medium
universal
physics
arxiv
2511.09468v1
https://arxiv.org/abs/2511.09468v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
9c5428fa02af41e11d270c3b00fdab99257960fe17fa360077e89e2314335042
Extracted from ArXiv paper 2511.09468v1 (chunk 0)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 0, "paper_id": "2511.09468v1" }
science
WO-ARX-01
2025-12-07T11:52:27.829675Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115235005288
The cross section values for the production of 11C, 13N, and 15O in proton-induced reactions on various targets were measured with improved precision.
The cross section values for the production of 11C, 13N, and 15O in proton-induced reactions on various targets were measured with improved precision.
[ "12C(p, d)11C reaction on natural carbon targets", "14N(p, d)13N reaction on BN targets", "16O(p, X) reactions on SiO2 wafers" ]
0.85
medium
universal
physics
arxiv
2511.09468v1
https://arxiv.org/abs/2511.09468v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
780d7cec2dcef0e80520218d42b5ce81cb52c55027bc5b235d5f24ff17f27c55
Extracted from ArXiv paper 2511.09468v1 (chunk 2)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 2, "paper_id": "2511.09468v1" }
science
WO-ARX-01
2025-12-07T11:52:35.005288Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115304673133
The observed supernova 1987A neutrino burst duration constrains new physics in the Lµ-Lτ boson sector, specifically limiting energy-loss mechanisms to LR = 4.4 × 10^52 erg/s.
The observed supernova 1987A neutrino burst duration constrains new physics in the Lµ-Lτ boson sector, specifically limiting energy-loss mechanisms to LR = 4.4 × 10^52 erg/s.
[ "Supernovae SN1987A", "Neutrino burst duration: ∼10 seconds", "Energy-loss constraint: LV (gµτ, mV ) ≤ LR" ]
0.85
high
universal
physics
arxiv
2511.09619v1
https://arxiv.org/abs/2511.09619v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
dfa67d7acffd829b3136e00d1af6ffbf0fa87ce1b4204b5ab96835439154a825
Extracted from ArXiv paper 2511.09619v1 (chunk 6)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 6, "paper_id": "2511.09619v1" }
science
WO-ARX-01
2025-12-07T11:53:04.673133Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115327816486
A peak in dijet invariant mass distribution is observed at M jj ≈0.95 TeV with a ∼3.4σ excess, consistent with the Θ → q¯q signal + background hypothesis.
A peak in dijet invariant mass distribution is observed at M jj ≈0.95 TeV with a ∼3.4σ excess, consistent with the Θ → q¯q signal + background hypothesis.
[ "CMS nonresonant analysis [21]", "M jj ∈[0.94, 1] TeV bin", "χ2 fit: χ2Θ+B = (24.1, 30.5, 7.7)" ]
0.85
high
universal
physics
arxiv
2511.09632v1
https://arxiv.org/abs/2511.09632v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
2d386c3ddd5d949742358fae7bb9cbb386c6ff22bcf1d3fe0c4ee52e8532b784
Extracted from ArXiv paper 2511.09632v1 (chunk 10)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 10, "paper_id": "2511.09632v1" }
science
WO-ARX-01
2025-12-07T11:53:27.816486Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115506385386
Topmetal-L detector achieves efficient readout of photoelectron tracks with approximately 176 pixels triggered per track, suitable for X-ray polarization analysis
Topmetal-L detector achieves efficient readout of photoelectron tracks with approximately 176 pixels triggered per track, suitable for X-ray polarization analysis
[ "40% He + 60% DME gas mixture at 1 atm", "5.90 keV X-rays from a 55Fe source", "step size < √Npixel ≈13.3 pixels" ]
0.85
medium
universal
physics
arxiv
2511.09863v2
https://arxiv.org/abs/2511.09863v2
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
7143e157f2501279954523c0b04c478a3eb5621d3544ab6166ecc0cb622cec11
Extracted from ArXiv paper 2511.09863v2 (chunk 11)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 11, "paper_id": "2511.09863v2" }
science
WO-ARX-01
2025-12-07T11:55:06.385386Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115521535569
A simulation study demonstrates the effectiveness of calibration and correction algorithms for the Polar-2/LPD detector.
A simulation study demonstrates the effectiveness of calibration and correction algorithms for the Polar-2/LPD detector.
[ "Polar-2/LPD detector", "Simulation data from [19] D. Yi et al.", "Calibration and correction algorithms improved detection accuracy by 15%" ]
0.85
medium
universal
physics
arxiv
2511.09863v2
https://arxiv.org/abs/2511.09863v2
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
c8fe1cc6e8a106fad9989e9f7b6d36b27c963a0e6b51082dbe9ce36511024542
Extracted from ArXiv paper 2511.09863v2 (chunk 16)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 16, "paper_id": "2511.09863v2" }
science
WO-ARX-01
2025-12-07T11:55:21.535569Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115527871874
A far detector placed along the beam line can collect a large fraction of LLP flux for specific ϕ decay modes, extending limits on exotic Higgs branching ratio.
A far detector placed along the beam line can collect a large fraction of LLP flux for specific ϕ decay modes, extending limits on exotic Higgs branching ratio.
[ "µTRISTAN experiment in µ+e−mode", "Highly asymmetric beams Eµ+ ≫Ee−", "Large cτϕ region with proper decay length" ]
0.85
high
universal
physics
arxiv
2511.10131v1
https://arxiv.org/abs/2511.10131v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
e401045f8c2eefcd91e3202de330acfa965d43890c07ff41488366896830fedb
Extracted from ArXiv paper 2511.10131v1 (chunk 0)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 0, "paper_id": "2511.10131v1" }
science
WO-ARX-01
2025-12-07T11:55:27.871874Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115543241833
Distributions of charged-hadron longitudinal momentum fraction, transverse momentum, and radial profile measured in beauty and charm jets at √s = 13 TeV.
Distributions of charged-hadron longitudinal momentum fraction, transverse momentum, and radial profile measured in beauty and charm jets at √s = 13 TeV.
[ "LHCb experiment", "Proton-proton collisions at √s = 13 TeV", "Beauty and charm jet distributions" ]
0.85
high
universal
physics
arxiv
2511.10216v1
https://arxiv.org/abs/2511.10216v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
b5aa7b3ff2e79eaf3a461f31cc7b76ceeffabed749a8afa0a60f7f0d96ab563a
Extracted from ArXiv paper 2511.10216v1 (chunk 0)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 0, "paper_id": "2511.10216v1" }
science
WO-ARX-01
2025-12-07T11:55:43.241833Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115554748216
The charged-hadron distributions in beauty- and charm-enhanced jets are measured with purities of 95% and 70-75%, respectively.
The charged-hadron distributions in beauty- and charm-enhanced jets are measured with purities of 95% and 70-75%, respectively.
[ "LHCb detector, 2023 data sample", "Beauty-enriched sample: 95% purity", "Charm-enriched sample: 70-75% purity" ]
0.85
medium
universal
physics
arxiv
2511.10216v1
https://arxiv.org/abs/2511.10216v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
3a38d36090880b1e81c12de59d7a46f66b7750a2e7916604c3bc6c1dc210a71f
Extracted from ArXiv paper 2511.10216v1 (chunk 4)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 4, "paper_id": "2511.10216v1" }
science
WO-ARX-01
2025-12-07T11:55:54.748216Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115625231771
Ratios of b-jet and c-jet distributions measured in beauty and charm jets compared to Z-tagged jets at √s = 8 TeV and √s = 13 TeV, with systematic uncertainties indicated.
Ratios of b-jet and c-jet distributions measured in beauty and charm jets compared to Z-tagged jets at √s = 8 TeV and √s = 13 TeV, with systematic uncertainties indicated.
[ "LHCb detector, 2023 data sample", "pp collisions at √s = 13 TeV, 1.6 fb^-1", "Z-tagged jets at √s = 8 TeV and √s = 13 TeV" ]
0.85
medium
universal
physics
arxiv
2511.10216v1
https://arxiv.org/abs/2511.10216v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
537613f70aa0aa9fc1470dcadc3cd5ad279e49bd45132c7afedb674413e2cac4
Extracted from ArXiv paper 2511.10216v1 (chunk 14)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 14, "paper_id": "2511.10216v1" }
science
WO-ARX-01
2025-12-07T11:56:25.231771Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115620142917
Significant strangeness enhancement trend observed in high-multiplicity proton–proton collisions at the LHC
Significant strangeness enhancement trend observed in high-multiplicity proton–proton collisions at the LHC
[ "ALICE detector, 2017 LHC data-taking campaign", "√s = 5.02 TeV, 2.3 nb−1 collected", "Highest multiplicity regime reached particle abundances comparable to central heavy-ion collisions" ]
0.85
high
universal
physics
arxiv
2511.10306v1
https://arxiv.org/abs/2511.10306v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
3e935b697ea2b56c39b95edfbd445e8b9208dce1f93abdfc8572e914d437ff41
Extracted from ArXiv paper 2511.10306v1 (chunk 1)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 1, "paper_id": "2511.10306v1" }
science
WO-ARX-01
2025-12-07T11:56:20.142917Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115646808280
The ALICE Time-Of-Flight detector achieves a time resolution of 100 ps with the 2022 data-taking statistics.
The ALICE Time-Of-Flight detector achieves a time resolution of 100 ps with the 2022 data-taking statistics.
[ "ALICE Time-Of-Flight detector, Run 3 data", "Time-over-threshold granularity: 12.5 ns", "Average interaction rate: 500 kHz" ]
0.85
medium
universal
physics
arxiv
2511.10311v1
https://arxiv.org/abs/2511.10311v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
bdb1045ec7257987df6c6ddad2cd59d4d0f4b39525421f8b5319052c3f447daa
Extracted from ArXiv paper 2511.10311v1 (chunk 5)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 5, "paper_id": "2511.10311v1" }
science
WO-ARX-01
2025-12-07T11:56:46.808280Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115650133747
Time resolution of the ALICE Time-Of-Flight detector in Run 3 is measured to be around 100 ps with non-Gaussian tail contribution accounting for 6% of the signal
Time resolution of the ALICE Time-Of-Flight detector in Run 3 is measured to be around 100 ps with non-Gaussian tail contribution accounting for 6% of the signal
[ "ALICE detector", "Two methods used: ∆∆tTOF and tTOF −texp −tFT0 ev", "EMG parameterization accounts for non-Gaussian effects" ]
0.85
medium
universal
physics
arxiv
2511.10311v1
https://arxiv.org/abs/2511.10311v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
428ff42274f1a6b99e5d04e3447bb457e01eda5bafaa486e8b82c3d060a90eb0
Extracted from ArXiv paper 2511.10311v1 (chunk 6)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 6, "paper_id": "2511.10311v1" }
science
WO-ARX-01
2025-12-07T11:56:50.133747Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115705913671
The ALICE Time-Of-Flight detector achieves time resolution of approximately 80.6 ps with a momentum range of 0.4 to 100 GeV/c.
The ALICE Time-Of-Flight detector achieves time resolution of approximately 80.6 ps with a momentum range of 0.4 to 100 GeV/c.
[ "ALICE detector", "13.6 TeV proton-proton collisions", "Time-of-flight method" ]
0.85
medium
universal
physics
arxiv
2511.10311v1
https://arxiv.org/abs/2511.10311v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
a213f26df00d6febf831c24a50c266d0d7c49c083acdd543488ae7df7ee950e8
Extracted from ArXiv paper 2511.10311v1 (chunk 11)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 11, "paper_id": "2511.10311v1" }
science
WO-ARX-01
2025-12-07T11:57:05.913671Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115715449376
Strong electromagnetic fields have been observed in ultra-peripheral collisions of heavy ions, where QED effects dominate and the Schwinger limit is approached.
Strong electromagnetic fields have been observed in ultra-peripheral collisions of heavy ions, where QED effects dominate and the Schwinger limit is approached.
[ "NA63 experiment at CERN", "200-GeV lepton beam", "Field strengths approaching the Schwinger limit" ]
0.85
high
universal
physics
arxiv
2511.10315v1
https://arxiv.org/abs/2511.10315v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
348db189038e665aa3fa76148a73c555595b4c25c132e086d12da554c7fbaad3
Extracted from ArXiv paper 2511.10315v1 (chunk 10)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 10, "paper_id": "2511.10315v1" }
science
WO-ARX-01
2025-12-07T11:57:15.449376Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115706855896
The 5/2+ state in 15Be decays mainly through the 14Beg.s.+n channel, but a small decay branch to the 14Be*(2+1) state is also observed.
The 5/2+ state in 15Be decays mainly through the 14Beg.s.+n channel, but a small decay branch to the 14Be*(2+1) state is also observed.
[ "Shell model analysis by (2015Fo04, 2018Fo07)", "Observed width of the proposed 5/2+ state by (2013Sn02) is 2σ larger than expected", "Decay to 14Be*(2+1) level predicted by (2015Fo04)" ]
0.85
medium
universal
physics
arxiv
2511.10321v1
https://arxiv.org/abs/2511.10321v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
b7a0f3a83cb5fed2fb693a62860d7d88244a9354fe52158a2e54a4c1c76fcfab
Extracted from ArXiv paper 2511.10321v1 (chunk 3)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 3, "paper_id": "2511.10321v1" }
science
WO-ARX-01
2025-12-07T11:57:06.855896Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115735529052
Invariant mass distributions for strange particles (K0S, Λ, Ξ−, Ω−) are measured in Pb–Pb collisions at √sNN = 5.02 TeV
Invariant mass distributions for strange particles (K0S, Λ, Ξ−, Ω−) are measured in Pb–Pb collisions at √sNN = 5.02 TeV
[ "ALICE detector data", "pT and centrality intervals", "signal extraction via Gaussian or Crystal-Ball fits to invariant mass distributions" ]
0.85
high
universal
physics
arxiv
2511.10360v1
https://arxiv.org/abs/2511.10360v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
54f32cba58728d342a61a042df312792e69448fea1b26b6941c6ed51c018be6a
Extracted from ArXiv paper 2511.10360v1 (chunk 5)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 5, "paper_id": "2511.10360v1" }
science
WO-ARX-01
2025-12-07T11:57:35.529577Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115738617289
Integrated yield of Λ baryons in Pb-Pb collisions at √sNN = 5.02 TeV measured with ALICE detector, within the 0-90% centrality class
Integrated yield of Λ baryons in Pb-Pb collisions at √sNN = 5.02 TeV measured with ALICE detector, within the 0-90% centrality class
[ "ALICE Collaboration, HIJING MC simulation", "Centrality: 0-90%", "pT interval: low and high ranges" ]
0.85
medium
universal
physics
arxiv
2511.10360v1
https://arxiv.org/abs/2511.10360v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
5285229277f1e2bfab29c9b9838cbe7dca4ba5a9adcb555996a036a9697fe467
Extracted from ArXiv paper 2511.10360v1 (chunk 6)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 6, "paper_id": "2511.10360v1" }
science
WO-ARX-01
2025-12-07T11:57:38.617822Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115734162381
Two-particle angular correlations in pp collisions at √s = 13 TeV show a peak around (∆y,∆ϕ) ≈(0,0), with deviations from unity observed due to trivial scaling effects.
Two-particle angular correlations in pp collisions at √s = 13 TeV show a peak around (∆y,∆ϕ) ≈(0,0), with deviations from unity observed due to trivial scaling effects.
[ "ALICE experiment", "2016, 2017, and 2018 data sample", "Signal distribution shows a triangular-shaped background in ∆y" ]
0.85
medium
universal
physics
arxiv
2511.10399v1
https://arxiv.org/abs/2511.10399v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
e94e1a2d411f7279b98a9432cd1101b43081880ac584657e0b02e50f4df06f20
Extracted from ArXiv paper 2511.10399v1 (chunk 3)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 3, "paper_id": "2511.10399v1" }
science
WO-ARX-01
2025-12-07T11:57:34.162381Z
arxiv
physics_recovered
arxiv_physics
w_20251207_115740491368
Two-particle angular correlations in pp collisions at √s = 13 TeV were studied with ALICE detector, achieving exceptional purity levels for pions and protons.
Two-particle angular correlations in pp collisions at √s = 13 TeV were studied with ALICE detector, achieving exceptional purity levels for pions and protons.
[ "ALICE detector, LHC run 2016-2018 data", "Pion purity: 99.5%", "Proton purity: 98%" ]
0.85
medium
universal
physics
arxiv
2511.10399v1
https://arxiv.org/abs/2511.10399v1
[ "hep-ex", "nucl-ex", "physics.atom-ph", "physics.plasm-ph", "astro-ph.HE" ]
cbae61bbc1edb77748dab3caa7af9955c9f32e9c45e63c21e4773229d0438ea6
Extracted from ArXiv paper 2511.10399v1 (chunk 5)
[ "experimental_physics", "measurement" ]
llama3.1:8b-instruct-q5_K_M
{ "ingested_by": "mneme", "version": "physics_mvpn_1.0", "contract": "WO-PHYS-03", "chunk_id": 5, "paper_id": "2511.10399v1" }
science
WO-ARX-01
2025-12-07T11:57:40.491368Z
arxiv
physics_recovered
arxiv_physics