File:Spectral density of GUE, N = 1 to 32.png
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Summary
| DescriptionSpectral density of GUE, N = 1 to 32.png |
English: Histogram of the spectral density of GUE(N), N = 1 to 32, sampled empirically, compared to theory (in black curves).
Matplotlib codeimport numpy as np
import matplotlib.pyplot as plt
from scipy.linalg import eigvalsh_tridiagonal # SciPy ≥ 1.15.3
from numpy.polynomial.hermite_e import hermeval
from math import factorial
# --------------------------------------------------------------------------
betas = [2]
Ns = [1, 2, 4, 8, 16, 32]
Nmatr = 100_000
window = 5
bins = 400
# --------------------------------------------------------------------------
def concat_batch_eigs(N: int, beta: int, m: int) -> np.ndarray:
size = m * N
d = np.random.randn(size) * np.sqrt(2.0 / beta)
e = np.zeros(size - 1)
if N > 1:
dfs = beta * np.tile(np.arange(1, N), m)
chi = np.random.chisquare(dfs)
e_int = np.sqrt(chi / beta)
mask = np.ones(size - 1, dtype=bool)
mask[np.arange(N - 1, size - 1, N)] = False
e[mask] = e_int
w = eigvalsh_tridiagonal(d, e, lapack_driver='sterf', check_finite=False)
return w / np.sqrt(N) # global scaling λ/√N
# --- finite-N
def scaled_density(x: np.ndarray, N: int) -> np.ndarray:
x = np.sqrt(N) * x
coef_Nm1 = np.zeros(N) ; coef_Nm1[-1] = 1.0
coef_N = np.zeros(N + 1) ; coef_N [-1] = 1.0
coef_Np1 = np.zeros(N + 2) ; coef_Np1[-1] = 1.0
He_Nm1 = hermeval(x, coef_Nm1)
He_N = hermeval(x, coef_N)
He_Np1 = hermeval(x, coef_Np1)
pref = np.sqrt(N) * np.exp(-0.5 * x**2) / (
np.sqrt(2 * np.pi) * factorial(N))
return pref * (He_N**2 - He_Np1 * He_Nm1)
# Simulate
Es = {}
for beta in betas:
for N in Ns:
print(f'β={beta}, N={N} (block dim = {N*Nmatr})')
Es[(N, beta)] = concat_batch_eigs(N, beta, Nmatr)
# Plot
leg = {2: 'GUE'}
cols = {2: 'tab:red'}
fig, axs = plt.subplots(2, 3, figsize=(18, 9))
for i, N in enumerate(Ns):
ax = axs[i // 3, i % 3]
beta = 2
xs = Es[(N, beta)]
# histogram
ax.hist(xs, bins=bins, density=True,
color=cols[beta], alpha=0.6)
# finite‑N theory curve
x_th = np.linspace(xs.min(), xs.max(), 1000)
ax.plot(x_th, scaled_density(x_th, N),
'k-', lw=1, alpha=0.6)
ax.set_title(f'N = {N}', fontsize=14)
ax.grid(True)
fig.suptitle(r'Spectral density of GUE with $W_N/\sqrt{N}$',
fontsize=18, y=1.02)
plt.tight_layout()
# plt.savefig('Spectral density GUE, N = 1 to 32.png')
plt.show()
|
| Date | |
| Source | Own work |
| Author | Cosmia Nebula |
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6 July 2025
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 03:39, 7 July 2025 | 1,790 × 922 (132 KB) | wikimediacommons>Cosmia Nebula | Uploaded while editing "Gaussian ensemble" on en.wikipedia.org |
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