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Spectral Form Factors and Ramp–Plateau Physics

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The spectral form factor separates correlations in a discrete energy spectrum from the smooth density of states. After unfolding and subtracting the disconnected contribution, a linear random-matrix ramp diagnoses long-range level correlations, while a late plateau reflects spectral discreteness. The dip of the full statistic is partly a competition with the decaying smooth-density term. None of these features alone uniquely identifies a wormhole, an ensemble ontology, or a particular microscopic theory.

Required background. Quantum Information supplies traces, ensemble averages, variance, and finite-sample estimators.

Helpful background. Semiclassical Gravity supplies Euclidean topology expansions; Quantum Fields in Curved Spacetime supplies thermal traces; Black-Hole Information supplies factorization and replica saddles; Quantum Gravity supplies the microscopic-interpretation problem.

For one Hamiltonian HH,

ZH(β+it)=Tr⁡e−(β+it)H.Z_H(\beta+it)=\operatorname{Tr}e^{-(\beta+it)H}.

An ensemble spectral form factor is

K(β,t)=⟨ZH(β+it)ZH(β−it)⟩.K(\beta,t) = \left\langle Z_H(\beta+it)Z_H(\beta-it) \right\rangle.

Its disconnected and connected pieces are

Kdisc=∣⟨ZH(β+it)⟩∣2,Kc=K−Kdisc.K_{\mathrm{disc}} = \left\lvert\left\langle Z_H(\beta+it)\right\rangle\right\rvert^2, \qquad K_{\mathrm c}=K-K_{\mathrm{disc}}.

KdiscK_{\mathrm{disc}} is largely fixed by the smooth one-point density. The correlation diagnostic is KcK_{\mathrm c} after energy unfolding, symmetry-sector separation, and a declared ensemble or time average. Cotler and collaborators distinguish slope, dip, ramp, and plateau and relate them to black-hole spectral questions in Cotler et al. 2017, §§2–4.

The plateau has a simple check independent of random-matrix theory. Expanding the product gives ∑i,je−β(Ei+Ej)e−it(Ei−Ej)\sum_{i,j}e^{-\beta(E_i+E_j)}e^{-it(E_i-E_j)}. For a discrete nondegenerate spectrum, an infinite-time average removes the terms with i≠ji\ne j, leaving ZH(2β)Z_H(2\beta). With degeneracy gEg_E, the answer is instead ∑EgE2e−2βE\sum_E g_E^2e^{-2\beta E}. Thus discreteness supplies a time-averaged plateau; correlations determine how the statistic approaches it. At β=0\beta=0, dividing by the number of retained nondegenerate levels gives the unit plateau used below.

The named generated dataset is GUE64-512-seed2207-v1. It contains 512 independent 64×6464\times64 complex Hermitian matrices in the Gaussian unitary ensemble, generated with PCG64 seed 2207. If XX has independent real and imaginary standard normal entries, the generator uses

H=X+X†264.H=\frac{X+X^\dagger}{2\sqrt{64}}.

The reference environment is CPython 3.11.9 and NumPy 2.0.2. An independent rerun with NumPy 2.3.5 agrees at the printed precision. No realizations or degeneracies were discarded; exact degeneracies, if encountered, would be retained. The full eigenvalue mean is 1.17864×10−41.17864\times10^{-4} and the calibrated second moment is 0.999719±0.0009520.999719\pm0.000952, consistent with the unit-variance semicircle normalization.

For each sorted spectrum, select indices 16 through 47: the central 32 levels. This fixed-count window discards 16 edge levels on each side. Unfold each retained eigenvalue EE using the theoretical semicircle cumulative distribution

ξ(E)=64[12+E4−E24π+arcsin⁡(E/2)π].\xi(E) =64\left[ \frac12 +\frac{E\sqrt{4-E^2}}{4\pi} +\frac{\arcsin(E/2)}{\pi} \right].

The observed retained range is −0.863718≤E≤0.863304-0.863718\le E\le0.863304. No empirical polynomial fit is used. With mean unfolded spacing one, define τ=t/tH\tau=t/t_{\mathrm H} and tH=2πt_{\mathrm H}=2\pi. The Fourier phase is e−2πiτξe^{-2\pi i\tau\xi}, consistent with the site convention e−iEte^{-iEt}.

This spectral unfolding removes the leading variation of the smooth mean density while preserving local ordering. It is a transformation with its own systematic uncertainty, not a harmless relabeling.

For realization ss with M=32M=32 retained levels, define

as(τ)=1M∑j=1Me−2πiτξsj.a_s(\tau) = \frac{1}{\sqrt M} \sum_{j=1}^{M}e^{-2\pi i\tau\xi_{sj}}.

The estimators are

K^=1512∑s∣as∣2,K^disc=∣1512∑sas∣2,K^c=K^−K^disc.\widehat K=\frac1{512}\sum_s\lvert a_s\rvert^2, \qquad \widehat K_{\mathrm{disc}} =\left\lvert\frac1{512}\sum_s a_s\right\rvert^2, \qquad \widehat K_{\mathrm c}=\widehat K-\widehat K_{\mathrm{disc}}.

Uncertainties are delete-one-realization jackknife standard errors for K^c\widehat K_{\mathrm c}. This plug-in connected estimator is the sample variance with denominator L=512L=512, so its expectation is (1−1/L)Kc(1-1/L)K_{\mathrm c}. Multiplying it by L/(L−1)L/(L-1) would remove that finite-sample bias. The table deliberately retains the estimator displayed above; its 1/512≃0.20%1/512\simeq0.20\% downward bias is smaller than the reported statistical errors and is not included in those error bars. The selected time grid was fixed before inspecting the results; all nine points are reported.

Scaled timeFull resultDisconnected resultConnected resultJackknife error
0.026.4981836.4696510.0285320.001269
0.051.2176841.1614900.0561940.002500
0.100.2091530.1011880.1079650.004427
0.200.2604690.0398780.2205920.009553
0.400.4115810.0024890.4090910.018618
0.700.6503250.0010450.6492810.027965
1.001.0702360.0046571.0655790.042607
1.500.9677890.0083940.9593940.042023
2.001.0307910.0033741.0274170.042150

The full statistic dips near τ=0.1\tau=0.1 as the disconnected piece decays. The connected values then track the GUE large-size benchmark Kc≃τK_{\mathrm c}\simeq\tau for 0<τ<10\lt\tau\lt1 and approach the unit plateau for τ≳1\tau\gtrsim1. The ramp, rather than the early smooth-density slope, is the feature diagnosing correlations beyond the one-point density. The deviation at τ=0.7\tau=0.7 is compatible with statistical uncertainty; this sample alone does not identify a finite-window or finite-NN systematic shift.

The principal finite-size limitation is that a 64-level matrix with only 32 retained levels has a short ramp and a noisy late-time plateau. Neither a pointwise unit plateau nor an exactly linear slope is expected in one finite sample. The fixed-count window also forces as(0)=Ma_s(0)=\sqrt M in every realization, so K^c(0)=0\widehat K_{\mathrm c}(0)=0 exactly. A Poisson comparison with the same window must respect this endpoint rather than demand an immediate unit value at τ=0\tau=0.

Save the following program as sff_gue64.py; it generates the matrices, performs the declared selection and unfolding, and emits both calibration and the table.

import numpy as np
SEED, SAMPLES, N, M = 2207, 512, 64, 32
TIMES = (0.02, 0.05, 0.10, 0.20, 0.40, 0.70, 1.00, 1.50, 2.00)
rng = np.random.default_rng(SEED)
x = (rng.normal(size=(SAMPLES, N, N))
+ 1j * rng.normal(size=(SAMPLES, N, N)))
h = (x + x.conj().transpose(0, 2, 1)) / (2.0 * np.sqrt(N))
all_levels = np.linalg.eigvalsh(h)
levels = all_levels[:, N // 4:3 * N // 4]
def semicircle_cdf(energy):
energy = np.clip(energy, -2.0, 2.0)
root = np.sqrt(np.maximum(0.0, 4.0 - energy * energy))
return (0.5 + energy * root / (4.0 * np.pi)
+ np.arcsin(energy / 2.0) / np.pi)
def connected_and_jackknife(amplitude):
power = np.abs(amplitude) ** 2
estimate = power.mean() - abs(amplitude.mean()) ** 2
leave_power = (power.sum() - power) / (SAMPLES - 1)
leave_mean = (amplitude.sum() - amplitude) / (SAMPLES - 1)
leave_connected = leave_power - np.abs(leave_mean) ** 2
error = np.sqrt((SAMPLES - 1) / SAMPLES
* np.sum((leave_connected - leave_connected.mean()) ** 2))
return estimate, error
unfolded = N * semicircle_cdf(levels)
second_moments = np.mean(all_levels ** 2, axis=1)
second_error = second_moments.std(ddof=1) / np.sqrt(SAMPLES)
print(f"mean={all_levels.mean():.8f} second={second_moments.mean():.8f} "
f"second_se={second_error:.8f}")
print("tau full disconnected connected jackknife_se")
for tau in TIMES:
amplitude = np.exp(-2j * np.pi * tau * unfolded).sum(axis=1) / np.sqrt(M)
full = np.mean(np.abs(amplitude) ** 2)
disconnected = abs(np.mean(amplitude)) ** 2
connected, error = connected_and_jackknife(amplitude)
print(f"{tau:.2f} {full:.6f} {disconnected:.6f} "
f"{connected:.6f} {error:.6f}")

Run python3 sff_gue64.py in that pinned environment. The matrix entries are generated data rather than a committed external dataset; seed, algorithm, parameters, transformation, selection, estimator, and output precision fully specify regeneration.

At τ=0.4\tau=0.4, repeating the same generator and central-half selection gives Kc=0.4154±0.0187K_{\mathrm c}=0.4154\pm0.0187 for N=32N=32 with 512 samples, 0.4091±0.01860.4091\pm0.0186 for N=64N=64 with 512 samples, and 0.4382±0.02690.4382\pm0.0269 for N=128N=128 with 256 samples. Their spread is consistent with finite-sample uncertainty; it is not evidence for an exact unit slope at these sizes.

Additional systematics are the central-window fraction, theoretical versus empirical unfolding, realization count, time binning, disconnected subtraction, and matrix symmetry class. GOE changes the universal ramp coefficient; mixing symmetry sectors can wash out level repulsion. A Poisson spectrum has no GUE linear connected ramp after proper averaging, while a picket-fence spectrum produces recurrences that can masquerade as a plateau on a short window.

The permissive gravitational interpretation associates the connected ramp with a Euclidean double-trumpet saddle, as in the JT/matrix relation Saad, Shenker, and Stanford 2019, §§2–5. A conservative interpretation calls the ramp evidence for universal correlated levels but not for a unique spacetime saddle. A single-sample interpretation obtains similar local statistics after time or energy smoothing without claiming a literal ensemble. These competing positions agree on the estimator but not its ontology; the inference remains unresolved.

Results and open questions as of 2026-08-19

Section titled “Results and open questions as of 2026-08-19”

The frontier cutoff is 2026-08-19.

Evidence or resultModel and analysis choiceLimitation or competing conclusion
Dip, ramp, and plateau in chaotic spectra, Cotler et al. 2017, §§2–4Random-matrix and selected many-body spectra with declared averagingFinite-size, smoothing, and disconnected-density artifacts must be separated
JT connected topology match, Saad, Shenker, and Stanford 2019, §§2–5Perturbative JT gravity and matrix-integral correlatorsEstablishes a controlled model, not a unique saddle interpretation for every theory
Symmetry-class dependence, Stanford and Witten 2020, §§2–5JT variants and random-matrix symmetry classesRamp coefficient and plateau structure depend on antiunitary symmetries and sectors

Useful adverse checks compare the result with a calculation that omits disconnected subtraction, or with independent levels drawn from the same smooth one-point density and processed with the same window and normalization. The first exposes the early smooth-density contribution; the second removes level correlations while preserving the density in expectation. Merely shuffling nearest-neighbor spacings is not a Poisson control: it retains their level-repulsion distribution and can leave nontrivial spectral correlations. Omitting unfolding is also not, by itself, an invalid calculation; it changes the statistic and requires comparison with an appropriately density-weighted theoretical prediction.

The conclusions could change after a larger named dataset changes the unfolded connected statistic beyond quoted finite-sample errors, after a controlled single-theory gravity calculation fixes the averaging prescription, or after a new saddle or symmetry sector changes the predicted ramp or plateau normalization.

At τ=0.40\tau=0.40, use the table to compute the fraction of the full result due to the disconnected term. Why would fitting the full value alone still be a poor test of the GUE ramp at τ=0.02\tau=0.02?

Solution

The fraction is 0.002489/0.411581≃0.006050.002489/0.411581\simeq0.00605, about 0.6%0.6\%, so the full and connected estimators nearly agree at τ=0.40\tau=0.40. At τ=0.02\tau=0.02, the disconnected contribution is 6.4696516.469651 out of 6.4981836.498183, about 99.6%99.6\%. The full early-time curve is therefore controlled by the smooth density, not the connected level correlations; fitting it as a ramp would test the wrong quantity.

  • Cotler et al. 2017, Jordan S. Cotler et al., “Black Holes and Random Matrices,” Journal of High Energy Physics 05 (2017) 118.
  • Saad, Shenker, and Stanford 2019, Phil Saad, Stephen H. Shenker, and Douglas Stanford, “JT Gravity as a Matrix Integral,” arXiv:1903.11115 (2019).
  • Stanford and Witten 2020, Douglas Stanford and Edward Witten, “JT Gravity and the Ensembles of Random Matrix Theory,” Advances in Theoretical and Mathematical Physics 24 (2020) 1475–1680.