{"total":13,"items":[{"citing_arxiv_id":"2605.16619","ref_index":4,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Evaporating Black Hole Interior and Complexity Evolution","primary_cat":"hep-th","submitted_at":"2026-05-15T20:41:21+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"In a JT gravity model with an EoW brane, black hole interior complexity grows linearly until the Page time then decays exponentially, with fluctuations growing large afterward and signaling loss of self-averaging.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.12468","ref_index":14,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Large $N$ factorization of families of tensor trace-invariants","primary_cat":"math-ph","submitted_at":"2026-05-12T17:52:03+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Families of complex tensor trace-invariants with tree-like dominant pairings factorize at large N, allowing computation of typical multipartite Rényi entropies for uniform random states.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"\"Tensor models and group field theories: combinatorics, largeNand renormalization\". In: Encyclpodia of Mathematical Physics, 2nd Edition(2025).doi:10.1016/B978- 0- 323- 95703- 8.00112- 9. arXiv:2404.07834 [math-ph]. [13] Don N. Page. \"Average entropy of a subsystem\". In:Phys. Rev. Lett.71 (1993), pp. 1291-1294.doi:10. 1103/PhysRevLett.71.1291. arXiv:gr-qc/9305007. [14] S. K. Foong and S. Kanno. \"Proof of Page's conjecture on the average entropy of a subsystem\". In:Phys. Rev. Lett.72 (8 1994), pp. 1148-1151.doi:10.1103/PhysRevLett.72.1148.url:https://link.aps.org/ doi/10.1103/PhysRevLett.72.1148. [15] Jorge S' anchez-Ruiz. \"Simple proof of Page's conjecture on the average entropy of a subsystem\". In:Phys. Rev. E52."},{"citing_arxiv_id":"2605.09783","ref_index":4,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Quantum Maxwell Demon at the Black Hole Horizon: Thermodynamics, Information, and the Equivalence Principle","primary_cat":"gr-qc","submitted_at":"2026-05-10T22:01:58+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"A quantum Maxwell demon near a black hole horizon loses some work extraction ability for external observers due to information inaccessibility but obeys local thermodynamics and preserves the equivalence principle for internal observers.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"paradox [1, 3], which demonstrates that accepting black hole complementarity together with three natural assumptions-(I) unitary evolution of black hole evaporation, (II) the - 1 - equivalence principle for infalling observers, and (III) the validity of effective quantum field theory for external observers-leads to a violation of the monogamy of entanglement [6, 7]. Specifically, late radiationBfrom an old black hole [4, 5], would need to be entan- gled simultaneously with early radiationR B and interior modesA, which is quantum- mechanically impossible. The AMPS proposal-that the entanglement betweenBandA breaks down, producing a firewall-highlights the tension between quantum mechanics, gravity, and thermodynamics near the horizon. The possible breakdown of the equivalence principle in the near-horizon region, and"},{"citing_arxiv_id":"2605.03015","ref_index":45,"ref_count":4,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The Fate of Nucleated Black Holes in de Sitter Quantum Gravity","primary_cat":"hep-th","submitted_at":"2026-05-04T18:00:08+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Nucleated black holes in de Sitter space evaporate via standard Hawking radiation back to the empty vacuum, rendering nucleation a temporary fluctuation.","context_count":2,"top_context_role":"background","top_context_polarity":"background","context_text":"Theor. Phys.83(1990) 1126-1139. [43] T. R. Choudhury and T. Padmanabhan, \"Concept of temperature in multi-horizon spacetimes: Analysis of Schwarzschild-de Sitter metric,\"Gen. Rel. Grav.39(2007) 1789-1811,arXiv:gr-qc/0404091. [44] D. A. Easson, \"The fate of Schwarzschild-de Sitter black holes: nonequilibrium evaporation,\"arXiv:2511.11873 [hep-th]. [45] D. N. Page, \"Average entropy of a subsystem,\"Phys. Rev. Lett.71(1993) 1291-1294, arXiv:gr-qc/9305007 [gr-qc]. [46] D. N. Page, \"Information in black hole radiation,\"Phys. Rev. Lett.71(1993) 3743-3746, arXiv:hep-th/9306083 [hep-th]. [47] D. N. Page, \"Time Dependence of Hawking Radiation Entropy,\"JCAP1309(2013) 028, arXiv:1301.4995 [hep-th]. - 59 -"},{"citing_arxiv_id":"2605.01887","ref_index":13,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Properties of tensorial free cumulants","primary_cat":"math-ph","submitted_at":"2026-05-03T14:06:15+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"The authors extend tensorial free cumulants to arbitrary orders, connect prior frameworks, and compute non-trivial examples for Gaussian tensors with structured covariances.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.26141","ref_index":1,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Typical entanglement entropy with charge conservation","primary_cat":"quant-ph","submitted_at":"2026-04-28T22:02:38+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Typical entanglement entropy with fixed global charge is given by the local thermal entropy at fixed charge density for both U(1) and SU(2) symmetries in the thermodynamic limit.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"3 Example:Nqutrits at fixed globalSU(2)charge (spin1) . . . . . . . . . . . 22 6.4 Example:Ntrimers of spin- 1 2 at fixedSU(2)charge . . . . . . . . . . . . . . 23 7 Discussion 24 A Laplace approximation and discontinuities 27 A.1Y 3 term . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 29 1 Introduction In a seminal paper [1] Page showed that, in aN-qubit system withN≫1, the typical entanglement entropy of aN A-qubit subsystem scales aslog(2)N A forN A < N/2. The coefficientlog(2)can be understood as the entropy of a single qubit at infinite temperature.1 ForasystemofNqubitsatfixedU(1)chargem, thetypicalentanglemententropywiththe charge constraint [2] is found to scale asη(s)NA, withs=m/Nandη(s) =− 1−2s"},{"citing_arxiv_id":"2604.12141","ref_index":34,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Quantum chaotic systems: a random-matrix approach","primary_cat":"quant-ph","submitted_at":"2026-04-13T23:44:23+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":0.0,"formal_verification":"none","one_line_summary":"Review of random matrix theory application to quantum chaos, covering symmetry classes, eigenvalue statistics, unfolding, and correlation functions.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Especially two developments should briefly mentioned here. Firstly, the eigenvector statistics of Hermitian Hamiltonians experience a revival in recent years due to the computation of quantum informational benchmarks, for instance in the investigation of many- body systems [196]. See the review [48] and book chapter [32]. Following the ideas of Lubkin [36], Lloyd and Pagels [33] and Page [34] of considering a uniformly distributed pure state the corresponding reduced density matrix becomes a random matrix called the fixed trace ensemble. In recent years, these ideas were generalised to more structured and physical Hilbert spaces, e.g., see [48, 47, 49, 197, 198]. The BGS conjecture [16] serves as an explanation to describe the eigenvectors of a quantum chaotic one-body Hamiltonian by a uniform"},{"citing_arxiv_id":"2604.09180","ref_index":8,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Eigenstate entanglement entropy in Bose-Hubbard models","primary_cat":"cond-mat.stat-mech","submitted_at":"2026-04-10T10:06:06+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"The volume-law coefficient of eigenstate entanglement entropy in Bose-Hubbard models remains unchanged by on-site disorder, while the O(1) contribution depends on particle density and bosonic cutoff in conserving cases and may become universal without conservation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2512.22997","ref_index":30,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Generalised Entanglement Entropies from Unit-Invariant Singular Value Decomposition","primary_cat":"hep-th","submitted_at":"2025-12-28T16:51:19+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Generalized entanglement entropies are constructed via left-, right-, and bi-invariant unit-invariant singular value decompositions to ensure scale invariance for non-Hermitian and rectangular operators in quantum mechanics, random matrices, and Chern-Simons theory.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2512.04318","ref_index":7,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Probing Evaporating Black Holes with Modular Flow in SYK","primary_cat":"hep-th","submitted_at":"2025-12-03T23:08:07+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Modular flow in SYK models coupled to a bath reveals singularities allowing reconstruction of bulk flow past the horizon in two-sided AdS2 black holes.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2411.01105","ref_index":16,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"UV Effects and Short-Lived Hawking Radiation: Alternative Resolution of Information Paradox","primary_cat":"hep-th","submitted_at":"2024-11-02T01:59:46+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Hawking radiation terminates around the scrambling time due to trans-Planckian stringy effects in GUP and string-field-theory-inspired toy models, yielding negligible evaporation and a mostly classical black hole.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Shao and C.T. Wang,Hawking radiation under generalized uncertainty principle, Eur. Phys. J. C83 (2023) 1118 [arXiv:2309.01638]. [14] P.M. Ho, Y. Imamura, H. Kawai and W.H. Shao,A stringy effect on Hawking radiation, JHEP 12 (2023) 122 [arXiv:2309.12926]. [15] D.N. Page,Information in black hole radiation, Phys. Rev. Lett.71 (1993) 3743 [hep-th/9306083]. [16] D.N. Page,Average entropy of a subsystem, Phys. Rev. Lett.71 (1993) 1291 [gr-qc/9305007]. [17] A. Almheiri, D. Marolf, J. Polchinski and J. Sully,Black Holes: Complementarity or Firewalls?, JHEP 02 (2013) 062 [arXiv:1207.3123]. [18] W.G. Unruh,Sonic analog of black holes and the effects of high frequencies on black hole evaporation, Phys. Rev. D51 (1995) 2827 [gr-qc/9409008]."},{"citing_arxiv_id":"1911.11977","ref_index":2,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Replica wormholes and the black hole interior","primary_cat":"hep-th","submitted_at":"2019-11-27T06:30:56+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":9.0,"formal_verification":"none","one_line_summary":"Replica wormhole geometries justify the replica trick computation of the Page curve in holographic black hole models and support entanglement wedge reconstruction via the Petz map.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"1905.08762","ref_index":45,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The entropy of bulk quantum fields and the entanglement wedge of an evaporating black hole","primary_cat":"hep-th","submitted_at":"2019-05-21T17:27:30+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":7.0,"formal_verification":"none","one_line_summary":"In a 2d evaporating black hole model, large boosts create O(1/G_N) gradients in bulk entropy that move the quantum extremal surface, causing the generalized entropy to follow unitary expectations with information disappearing after a scrambling time and a phase transition at the Page time.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}