Notes on Wasserstein distance and the JT gravitational ensemble

Primarily AI-generated textHuman understanding: some partsmath-ph — Mathematical Physicsmath.PR — Probabilityquant-ph — Quantum Physics

Contributed by Ville Samuli Keränen ↗

Version 1 / Nov 11, 2026 / CC BY 4.0

Abstract

This note completes the study of the Boltzmann–Wasserstein (BW) distance, an optimal-transport metric on quantum theories, begun in a companion paper (arXiv:2606.01296). There the distance was evaluated between macroscopically different theories; here we take the opposite limit, two independent draws of the JT-gravity ensemble, which are identical at the classical level. The distance is computable and is controlled by the connected spectral form factor: the ramp, the double-trumpet wormhole, regulated by the plateau, the spectral discreteness. The mean is exponentially small, ⟨W2⟩∼S0 e−S0\langle \mathcal{W}^2\rangle \sim S_0\, e^{-S_0}, whereas uncorrelated (Poisson) levels would give an unsuppressed O(1)O(1) distance: the self-distance is a sharp diagnostic of spectral chaos. As a metric, the BW distance renders the ensemble a point cloud: exponentially small, strongly anisotropic, its leading principal axis a coherent “breathing” deformation of the low-energy spectrum. Its effective dimension grows asymptotically as Deff≃0.42 S02D_{\mathrm{eff}} \simeq 0.42\, S_0^2, so the distance self-averages, its relative width shrinking as std/mean∼1/S0\mathrm{std}/\mathrm{mean} \sim 1/S_0. At low temperatures it localizes on the Airy edge, where a single Tracy–Widom mode dominates and self-averaging fails. We test the picture with exact-diagonalization GUE and SYK simulations: in GUE the effective dimension grows logarithmically at every temperature and is predicted at finite NN, with no free parameters, by the same covariance; unfolded SYK exhibits the predicted anisotropy and mode structure of the cloud. Together with the companion result, this fixes the resolution of the metric: the microstate rigidity computed here is the noise floor beneath a macroscopic difference between theories.

Provenance statement

This work was produced in a back-and-forth collaboration between VK and Claude (Anthropic; models Opus 4.8 and Fable 5). Claude did the calculations and the writing first; VK checked the main-text calculations by hand or by independent simulation and rewrote parts of the text. The appendix numerics (exact diagonalization of SYK and GUE) are Claude’s, cross-checked internally but not by hand. The manuscript was reviewed in several passes by referee-prompted Claude agents and by Claude Fable 5.2 in a separate session; that review contributed one quantitative correction, which the authors then reproduced. A detailed account, including the limits of the review, is in the paper’s closing “Note on the preparation of this work.”

Tools used

Anthropic
Claude FableVersion 5
Anthropic
Claude FableVersion 5.2
Anthropic
Claude OpusVersion 4.8

References

  1. V. Keranen, Notes on Wasserstein distance and wormholes , arXiv:2606.01296.arXiv
  2. P. Saad, S. Shenker, D. Stanford, JT gravity as a matrix integral , arXiv:1903.11115.arXiv
  3. D. Marolf, H. Maxfield, Transcending the ensemble: baby universes, spacetime wormholes, and the order and disorder of black hole information , JHEP 08 (2020) 044, arXiv:2002.08950.arXiv
  4. P. Saad, S.H. Shenker, D. Stanford, A semiclassical ramp in SYK and in gravity , arXiv:1806.06840.arXiv
  5. P. Saad, Late time correlation functions, baby universes, and ETH in JT gravity , arXiv:1910.10311.arXiv
  6. C.V. Johnson, Nonperturbative Jackiw--Teitelboim gravity , Phys. Rev. D 101 (2020) 106023, arXiv:1912.03637.arXiv
  7. C.V. Johnson, Explorations of nonperturbative Jackiw--Teitelboim gravity and supergravity , arXiv:2006.10959.arXiv
  8. C.V. Johnson, Quantum gravity microstates from Fredholm determinants , Phys. Rev. Lett. 127 (2021) 181602, arXiv:2106.09048.arXiv
  9. C.V. Johnson, The microstate physics of JT gravity and supergravity , arXiv:2201.11942.arXiv
  10. K. Okuyama, K. Sakai, JT gravity, KdV equations and macroscopic loop operators , JHEP 01 (2020) 156, arXiv:1911.01659.arXiv
Show all 65 referencesShow fewer references
  1. A. Altland, J. Sonner, Late time physics of holographic quantum chaos , SciPost Phys. 11 (2021) 034, arXiv:2008.02271.arXiv
  2. A. Altland, B. Post, J. Sonner, J. van der Heijden, E.P. Verlinde, Quantum chaos in 2D gravity , SciPost Phys. 15 (2023) 064, arXiv:2204.07583.arXiv
  3. C. Villani, Optimal Transport: Old and New , Springer (2009).
  4. G. De Palma, D. Trevisan, Quantum optimal transport with quantum channels , Ann. Henri Poincaré 22 (2021) 3199, arXiv:1911.00803.arXiv
  5. G. De Palma, D. Trevisan, Quantum optimal transport: quantum channels and qubits , in Optimal Transport on Quantum Structures , Springer (2024), arXiv:2307.16268.arXiv
  6. K. Hashimoto, N. Tanahashi, Holography and optimal transport: emergent Wasserstein spacetime in harmonic oscillator, SYK and Krylov complexity , arXiv:2604.17649.arXiv
  7. K. Hashimoto, N. Tanahashi, K. Yoshida, Wasserstein space of quantum chaos , arXiv:2605.20995.arXiv
  8. A. Blommaert, T.G. Mertens, H. Verschelde, Eigenbranes in Jackiw--Teitelboim gravity , JHEP 02 (2021) 168, arXiv:1911.11603.arXiv
  9. O. Costin, J.L. Lebowitz, Gaussian fluctuation in random matrices , Phys. Rev. Lett. 75 (1995) 69.
  10. A. Soshnikov, Gaussian fluctuation for the number of particles in Airy, Bessel, sine, and other determinantal random point fields , J. Stat. Phys. 100 (2000) 491.
  11. J. Gustavsson, Gaussian fluctuations of eigenvalues in the GUE , Ann. Inst. H. Poincaré 41 (2005) 151.
  12. K. Johansson, On fluctuations of eigenvalues of random Hermitian matrices , Duke Math. J. 91 (1998) 151.
  13. C.A. Tracy, H. Widom, Level-spacing distributions and the Airy kernel , Commun. Math. Phys. 159 (1994) 151.
  14. M.V. Berry, Semiclassical theory of spectral rigidity , Proc. R. Soc. Lond. A 400 (1985) 229.
  15. M.L. Mehta, Random Matrices , 3rd ed., Elsevier (2004).
  16. B.L. Altshuler, B.I. Shklovskii, Repulsion of energy levels and conductivity of small metal samples , Sov. Phys. JETP 64 (1986) 127.
  17. I.S. Gradshteyn, I.M. Ryzhik, Table of Integrals, Series, and Products , 7th ed., Academic Press (2007), Eq. 6.693.2.
  18. M.V. Berry, M. Tabor, Level clustering in the regular spectrum , Proc. R. Soc. Lond. A 356 (1977) 375.
  19. P. Deift, A. Its, I. Krasovsky, Asymptotics of Toeplitz, Hankel, and Toeplitz+Hankel determinants with Fisher--Hartwig singularities , Ann. of Math. 174 (2011) 1243, arXiv:0905.0443.arXiv
  20. A.G. Abanov, D.A. Ivanov, Y. Qian, Quantum fluctuations of one-dimensional free fermions and Fisher--Hartwig formula for Toeplitz determinants , J. Phys. A 44 (2011) 485001, arXiv:1108.1355.arXiv
  21. S. Dallaporta, Eigenvalue variance bounds for Wigner and covariance random matrices , Random Matrices Theory Appl. 1 (2012) 1250007, arXiv:1203.1597.arXiv
  22. E.S. Meckes, M.W. Meckes, Concentration and convergence rates for spectral measures of random matrices , Probab. Theory Relat. Fields 156 (2013) 145, arXiv:1109.5997.arXiv
  23. R.E. Prange, The spectral form factor is not self-averaging , Phys. Rev. Lett. 78 (1997) 2280.
  24. K. Karhunen, Über lineare Methoden in der Wahrscheinlichkeitsrechnung , Ann. Acad. Sci. Fenn. Ser. A. I. Math.-Phys. 37 (1947) 1.
  25. M. Loève, Probability Theory II , 4th ed., Graduate Texts in Mathematics 46 , Springer (1978), Ch. X.
  26. O. Bohigas, M.J. Giannoni, C. Schmit, Characterization of chaotic quantum spectra and universality of level fluctuation laws , Phys. Rev. Lett. 52 (1984) 1.
  27. P.J. Forrester, The spectrum edge of random matrix ensembles , Nucl. Phys. B 402 (1993) 709.
  28. I. Dumitriu, A. Edelman, Matrix models for beta ensembles , J. Math. Phys. 43 (2002) 5830, arXiv:math-ph/0206043.arXiv
  29. J.A. Ramírez, B. Rider, B. Virág, Beta ensembles, stochastic Airy spectrum, and a diffusion , J. Amer. Math. Soc. 24 (2011) 919, arXiv:math/0607331.arXiv
  30. F. David, Phases of the large-NN matrix model and non-perturbative effects in 2d gravity , Nucl. Phys. B 348 (1991) 507.
  31. S.H. Shenker, The strength of nonperturbative effects in string theory , in Random Surfaces and Quantum Gravity (Cargèse 1990), Plenum (1991).
  32. V. Fateev, A.B. Zamolodchikov, Al.B. Zamolodchikov, Boundary Liouville field theory I. Boundary state and boundary two-point function , arXiv:hep-th/0001012.arXiv
  33. J. Teschner, Remarks on Liouville theory with boundary , arXiv:hep-th/0009138.arXiv
  34. S.N. Majumdar, G. Schehr, Top eigenvalue of a random matrix: large deviations and third-order phase transition , J. Stat. Mech. (2014) P01012, arXiv:1311.0580.arXiv
  35. S. Sachdev, J. Ye, Gapless spin-fluid ground state in a random quantum Heisenberg magnet , Phys. Rev. Lett. 70 (1993) 3339, arXiv:cond-mat/9212030.arXiv
  36. A. Kitaev, A simple model of quantum holography , KITP seminars, April and May 2015.
  37. J. Maldacena, D. Stanford, Remarks on the Sachdev--Ye--Kitaev model , Phys. Rev. D 94 (2016) 106002, arXiv:1604.07818.arXiv
  38. J.S. Cotler, G. Gur-Ari, M. Hanada, J. Polchinski, P. Saad, S.H. Shenker, D. Stanford, A. Streicher, M. Tezuka, Black holes and random matrices , arXiv:1611.04650.arXiv
  39. H. Gharibyan, M. Hanada, S.H. Shenker, M. Tezuka, Onset of random matrix behavior in scrambling systems , arXiv:1803.08050.arXiv
  40. E. Witten, Matrix models and deformations of JT gravity , Proc. R. Soc. Lond. A 476 (2020) 20200582, arXiv:2006.13414.arXiv
  41. H. Maxfield, G.J. Turiaci, The path integral of 3D gravity near extremality; or, JT gravity with defects as a matrix integral , JHEP 01 (2021) 118, arXiv:2006.11317.arXiv
  42. J. Pollack, M. Rozali, J. Sully, D. Wakeham, Eigenstate thermalization and disorder averaging in gravity , Phys. Rev. Lett. 125 (2020) 021601, arXiv:2002.02971.arXiv
  43. A. Belin, J. de Boer, Random statistics of OPE coefficients and Euclidean wormholes , Class. Quantum Grav. 38 (2021) 164001, arXiv:2006.05499.arXiv
  44. J. Chandra, S. Collier, T. Hartman, A. Maloney, Semiclassical 3D gravity as an average of large-cc CFTs , JHEP 12 (2022) 069, arXiv:2203.06511.arXiv
  45. P. Saad, S.H. Shenker, D. Stanford, S. Yao, Wormholes without averaging , JHEP 09 (2024) 133, arXiv:2103.16754.arXiv
  46. L.V. Iliesiu, G.J. Turiaci, The statistical mechanics of near-extremal black holes , arXiv:2003.02860.arXiv
  47. N. Benjamin, H. Ooguri, S.-H. Shao, Y. Wang, Light-cone modular bootstrap and pure gravity , Phys. Rev. D 100 (2019) 066029, arXiv:1906.04184.arXiv
  48. S. Collier, L. Eberhardt, M. Zhang, Solving 3d gravity with Virasoro TQFT , SciPost Phys. 15 (2023) 151, arXiv:2304.13650; S. Collier, L. Eberhardt, B. Mühlmann, V.A. Rodriguez, The Virasoro minimal string , SciPost Phys. 16 (2024) 057, arXiv:2309.10846.arXiv
  49. G. Di Ubaldo, E. Perlmutter, AdS3_3/RMT2_2 duality , arXiv:2307.03707; J. Boruch, G. Di Ubaldo, F.M. Haehl, E. Perlmutter, M. Rozali, Modular-invariant random matrix theory and AdS3_3 wormholes , Phys. Rev. Lett. 135 (2025) 121602, arXiv:2503.00101.arXiv
  50. D.L. Jafferis, L. Rozenberg, D. Sarkar, D. Wang, On random matrix statistics of 3d gravity , arXiv:2512.05045.arXiv
  51. Y.-Z. You, A.W.W. Ludwig, C. Xu, Sachdev--Ye--Kitaev model and thermalization on the boundary of many-body localized fermionic symmetry-protected topological states , Phys. Rev. B 95 (2017) 115150, arXiv:1602.06964.arXiv
  52. A.M. García-García, J.J.M. Verbaarschot, Spectral and thermodynamic properties of the Sachdev--Ye--Kitaev model , Phys. Rev. D 94 (2016) 126010, arXiv:1610.03816.arXiv
  53. V. Oganesyan, D.A. Huse, Localization of interacting fermions at high temperature , Phys. Rev. B 75 (2007) 155111, arXiv:cond-mat/0610854.arXiv
  54. Y.Y. Atas, E. Bogomolny, O. Giraud, G. Roux, Distribution of the ratio of consecutive level spacings in random matrix ensembles , Phys. Rev. Lett. 110 (2013) 084101, arXiv:1212.5611.arXiv
  55. Y. Jia, J.J.M. Verbaarschot, Spectral fluctuations in the Sachdev--Ye--Kitaev model , arXiv:1912.11923.arXiv

Version history

  1. v1 · 37 pagesSubmitted by Ville Samuli KeränenInitial depositCurrentNov 10, 2026