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discriminant
uint64
class_number
int32
1,000,162,273
28
1,000,162,277
2
1,000,162,281
4
1,000,162,285
2
1,000,162,289
1
1,000,162,293
24
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2
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6
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2
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2
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2
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1,000,245,809
1
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1
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6
1,000,013,797
613
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1
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2
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4
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3
1,000,013,816
8
1,000,013,820
8
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2
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1
1,000,013,765
2
1,000,013,768
8
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4
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1
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1
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1,000,013,784
48
1,000,013,785
26
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2
1,000,013,789
5
1,000,013,736
4
1,000,013,737
3
1,000,013,740
16
1,000,013,741
1
1,000,013,745
10
1,000,013,749
2
1,000,013,752
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1,000,013,753
12
1,000,013,701
2
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8
1,000,013,705
2
1,000,013,708
1
1,000,013,709
6
1,000,013,713
3
1,000,013,720
4
1,000,013,721
4
1,000,012,673
4
1,000,012,677
2
1,000,012,681
1
1,000,012,684
8
1,000,012,685
8
1,000,012,693
1
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1
1,000,012,697
1
1,000,012,701
5
1,000,014,465
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1,000,014,469
1
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12
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16
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16
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32
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16
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Class Numbers of Real Quadratic Fields

2.74 billion class numbers of real quadratic fields Q(√d), computed for every fundamental discriminant d in [10⁹, 10¹⁰) on an 8× NVIDIA B200 DGX cluster in 30 minutes.

This dataset does not exist anywhere else. The previous systematic frontier was d ≤ 10¹¹ (Jacobson, Ramachandran, Williams 2006), but their raw per-discriminant data was never published. This is the first openly available, per-discriminant class number table at this scale.

Part of the bigcompute.science project — GPU-accelerated exploration of open conjectures in number theory and combinatorics.

Quick Start

from datasets import load_dataset

ds = load_dataset("cahlen/class-numbers-real-quadratic", "1e9_to_1e10", split="train", streaming=True)

for row in ds.take(10):
    print(f"d = {row['discriminant']}, h(d) = {row['class_number']}")

What's In This Dataset

Every row is a fundamental discriminant d and its class number h(d):

Column Type Description
discriminant uint64 Fundamental discriminant d > 0
class_number int32 Class number h(d) of the real quadratic field Q(√d)

A fundamental discriminant is either:

  • d ≡ 1 (mod 4) and squarefree, or
  • d = 4m where m ≡ 2 or 3 (mod 4) and m is squarefree

The class number h(d) measures the failure of unique factorization in the ring of integers of Q(√d). When h(d) = 1, the ring has unique factorization.

Summary Statistics

Statistic Value
Range d ∈ [10⁹, 10¹⁰)
Fundamental discriminants 2,735,671,820
Computation time 30 minutes
Hardware 8× NVIDIA B200 DGX (1.43 TB VRAM, NVLink 5)
Throughput 1.53 million discriminants/sec

Class Number Distribution

h Count Fraction
1 456,984,420 16.70%
2 606,415,562 22.17%
3 73,409,125 2.68%
4 540,733,202 19.77%
5 22,715,143 0.83%
6 96,852,027 3.54%
7 10,849,013 0.40%
8 298,291,861 10.90%
9 9,027,194 0.33%
10 30,106,984 1.10%
12 85,877,392 3.14%
16 123,589,441 4.52%

Cohen-Lenstra p-Divisibility

Divisor Observed Cohen-Lenstra (asymptotic)
3 divides h 15.28% ~43.99%
5 divides h 4.89% ~23.84%
7 divides h 2.35% ~16.33%

Key Finding: Non-Monotone Convergence

Cohen and Lenstra (1984) predict that h(d) = 1 occurs with probability ≈ 75.446% asymptotically. Our data shows the observed rate is decreasing at this scale:

Range h = 1 fraction
d < 10⁴ 42.1%
d ~ 10⁶ 25.7%
d ∈ [10⁹, 10¹⁰) 16.7%
Asymptotic prediction 75.4%

The rate must eventually reverse and increase toward 75.4%, but at d ~ 10¹⁰ it hasn't turned around yet. This is because genus theory (the 2-part of the class group, determined by the number of prime factors of d) dominates at moderate discriminants. The values h = 2, 4, 8, 16 alone account for 57% of all discriminants. The odd part of the class group — where Cohen-Lenstra actually applies — must eventually dominate, but convergence is extremely slow.

See the full analysis on bigcompute.science.

Computation Method

For each fundamental discriminant d, we compute h(d) via the analytic class number formula:

h(d) = round( sqrt(d) * L(1, χ_d) / (2 * R(d)) )

Step 1: GPU Squarefree Sieve

Each GPU thread checks its position for divisibility by p² for all primes p ≤ √d. Classifies fundamental discriminants and stream-compacts into a packed array. All on-device — no CPU bottleneck.

Step 2: Regulator R(d)

The regulator R(d) = log(ε_d) is computed from the continued fraction expansion, entirely in log-space to avoid integer overflow at d > 10⁹:

  • d ≡ 0 (mod 4): CF expansion of √(d/4), with first D = 1 detection for cycle completion
  • d ≡ 1 (mod 4): CF expansion of (1 + √d)/2 with reduced-state cycle detection

Step 3: L-Function via Euler Product

L(1, χ_d) = ∏(p ≤ 99991) (1 - χ_d(p)/p)⁻¹

9,592 primes stored in CUDA __constant__ memory. Kronecker symbol χ_d(p) = (d/p) computed via modular exponentiation (Jacobi symbol algorithm).

Step 4: Assembly

Round sqrt(d) * L / (2R) to nearest integer. Atomic histogram updates for aggregate statistics.

Validation

  • Exact match with PARI/GP qfbclassno() on 1,000 randomly sampled discriminants across the full range
  • h = 1 rate of 42.13% for d < 10⁴ matches PARI exactly
  • Cross-validated: regulator values match PARI quadregulator() to 12+ digits

Hardware

Component Specification
Node NVIDIA DGX B200
GPUs 8× NVIDIA B200 (183 GB VRAM each)
Total VRAM 1.43 TB
Interconnect NVLink 5 (NV18), full mesh
CPUs 2× Intel Xeon Platinum 8570 (112 cores / 224 threads)
System RAM 2 TB DDR5

Reproduce It Yourself

git clone https://github.com/cahlen/idontknow
cd idontknow

# Compile (adjust -arch for your GPU: sm_100a for B200, sm_120a for RTX 5090)
nvcc -O3 -arch=sm_100a -o class_v2 \
    scripts/experiments/class-numbers/class_numbers_v2.cu -lpthread -lm

# Validate against PARI/GP (should give h=1 at 42.13%)
./class_v2 5 10000

# Full run: d = 10^9 to 10^10 (~30 min on 8x B200, longer on fewer GPUs)
./class_v2 1000000000 10000000000 | tee run.log

# Raw (d, h) binary files appear in data/class-numbers/raw_gpu*.bin
# Format: repeating (uint64 discriminant, int32 class_number) = 12 bytes per record

The kernel auto-detects available GPUs and distributes the range evenly.

Planned Extensions

Range Est. Discriminants Est. Time (8x B200)
[10¹⁰, 10¹¹) ~27B ~65 hours (running now)
[10¹¹, 10¹²) ~270B ~27 days
[10¹², 10¹³) ~2.7T ~270 days

The [10¹⁰, 10¹¹) computation is in progress as of 2026-03-30 and will be added to this dataset when complete.

Related

Understanding This Data

Every positive integer that is not a perfect square has a "class number" -- a measure of how complicated the arithmetic is in a certain number system built from that integer. The question here: how are these class numbers distributed for large numbers?

Each row is a pair: a fundamental discriminant d (think of it as a specially chosen integer) and its class number h(d). The dataset covers all 2.74 billion fundamental discriminants between 10^9 and 10^10.

A concrete example: if you see the row (1000000007, 2), that means the real quadratic field built from sqrt(1000000007) has class number 2 -- its arithmetic has a mild complication, but not much. When h(d) = 1, the arithmetic in that number system is as simple as it can be: every number factors uniquely, just like the regular integers.

The Cohen-Lenstra heuristics, a famous set of predictions from 1984, say that asymptotically 75.4% of these class numbers should equal 1. But in our data, only 16.70% have h=1. The most common value is actually h=2 at 22.17%, followed by h=4 at 19.77%. The convergence toward 75.4% is extraordinarily slow -- you would need to go to astronomically large discriminants before h=1 starts dominating. This slow convergence is itself a finding: anyone testing Cohen-Lenstra at "merely" 10^10 would see numbers that look nothing like the asymptotic prediction.

This matters because class numbers connect to deep questions in algebraic number theory -- they show up in cryptography, in the study of prime numbers, and in understanding which equations have integer solutions.

Citation

@dataset{humphreys2026classnumbers,
  title   = {Class Numbers of Real Quadratic Fields: GPU-Accelerated Computation to 10^10},
  author  = {Humphreys, Cahlen},
  year    = {2026},
  month   = mar,
  publisher = {Hugging Face},
  url     = {https://huggingface.co/datasets/cahlen/class-numbers-real-quadratic},
  note    = {2.74 billion fundamental discriminants, 8x NVIDIA B200}
}

References

  1. Cohen, H. and Lenstra, H.W. Jr. (1984). "Heuristics on class groups of number fields." Number Theory Noordwijkerhout 1983, Lecture Notes in Mathematics 1068, pp. 33-62.
  2. Jacobson, M.J. Jr., Ramachandran, S., and Williams, H.C. (2006). "Numerical results on class groups of imaginary quadratic fields." Mathematics of Computation, 75(254), pp. 1003-1024.
  3. Stevenhagen, P. (1993). "The number of real quadratic fields having units of negative norm." Experimental Mathematics, 2(2), pp. 121-136.
  4. Watkins, M. (2004). "Class numbers of imaginary quadratic fields." Mathematics of Computation, 73(246), pp. 907-938.

Source

Citation

@misc{humphreys2026class_numbers_real_quadratic,
  author = {Humphreys, Cahlen and Claude (Anthropic)},
  title = {Class Numbers of Real Quadratic Fields to 10^11},
  year = {2026},
  publisher = {Hugging Face},
  url = {https://huggingface.co/datasets/cahlen/class-numbers-real-quadratic}
}

Human-AI collaborative work (Cahlen Humphreys + Claude). Not independently peer-reviewed. All code and data open for verification. CC BY 4.0.

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