{"total":14,"items":[{"citing_arxiv_id":"2607.08737","ref_index":11,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The mini-Page Curve in Cosmology","primary_cat":"hep-th","submitted_at":"2026-07-09T17:37:03+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":6.5,"formal_verification":"none","one_line_summary":"In 2D centaur geometries the entropy difference of a modular-conjugate Hawking-pair probe traces an inverse mini-Page curve that bottoms at τ≈β/8, marking when information begins to leave the cosmological horizon.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2607.08661","ref_index":43,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The Remnant of an Evaporating Rotating Regular Black Hole from the Generalized Entropy in the Final Stage of Evaporation","primary_cat":"hep-th","submitted_at":"2026-07-09T16:28:23+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":5.0,"formal_verification":"none","one_line_summary":"A rotating regular black hole leaves a remnant because the correction term in the generalized entropy of Hawking radiation vanishes at a finite mass above the extremal limit.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.30797","ref_index":64,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"On Black Holes Surrounded by Radiation II: Thermodynamics","primary_cat":"hep-th","submitted_at":"2026-06-29T18:21:28+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Hillingar black holes thermodynamically mimic ordinary black holes of mass M, sharing temperature and entropy under thermal equilibrium.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.09346","ref_index":20,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Asymptotic Algebras and Holography of Information in CGHS Model","primary_cat":"hep-th","submitted_at":"2026-06-08T11:15:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Establishes holography of information in the CGHS model via asymptotic algebras and argues that islands violate commutativity of left- and right-boundary algebras.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.08347","ref_index":13,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Entanglement islands, fuzzballs and stretched horizons","primary_cat":"hep-th","submitted_at":"2026-05-08T18:01:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Fuzzball models with stretched horizons modify or eliminate entanglement islands depending on boundary conditions and cap geometry, producing information paradox analogues in some cases.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"[10] S.D. Mathur,The Fuzzball proposal for black holes: An Elementary review,Fortsch. Phys.53(2005) 793 [hep-th/0502050]. [11] I. Bena and N.P. Warner,Black holes, black rings and their microstates,Lect. Notes Phys.755(2008) 1 [hep-th/0701216]. [12] I. Bena and N.P. Warner,Resolving the Structure of Black Holes: Philosophizing with a Hammer,1311.4538. [13] A. Almheiri, R. Mahajan and J. Maldacena,Islands outside the horizon, 1910.11077. [14] H.Z. Chen, R.C. Myers, D. Neuenfeld, I.A. Reyes and J. Sandor,Quantum Extremal Islands Made Easy, Part I: Entanglement on the Brane,JHEP10(2020) 166 [2006.04851]. [15] H.Z. Chen, R.C. Myers, D. Neuenfeld, I.A. Reyes and J. Sandor,Quantum Extremal Islands Made Easy, Part II: Black Holes on the Brane,JHEP12(2020) 025"},{"citing_arxiv_id":"2604.26600","ref_index":12,"ref_count":2,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Entanglement Revivals and Scrambling for Evaporating Black Holes","primary_cat":"hep-th","submitted_at":"2026-04-29T12:29:23+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Entanglement revivals in evaporating black holes survive only when radiation intervals are larger than a critical length set by the exponential of the black-hole scrambling time.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"the partner modes enterA L YA R after reflection from the boundary mirror. We will examine below how the picture above is affected by the finite scrambling time of the black hole. Across the two setups - the AdS 2 black hole within JT 1The extra factor ofcin the argument of the log arises from the fact that there arecCFT degrees of freedom and thereforet scr is correspondingly shorter [12]. 2For simplicity, we consider only the symmetric case i.e. when the intervalsA L andA R are identical. - 2 - gravity , and asympotically flat black hole in the RST model - we find that the mutual information spike is smoothed out and reduced by the black hole scrambling effect, disappearing entirely below a critical value of the interval size, Lcrit \"c 1"},{"citing_arxiv_id":"2604.20165","ref_index":5,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Entropy bound and the non-universality of entanglement islands","primary_cat":"hep-th","submitted_at":"2026-04-22T04:10:59+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Universal compact entanglement islands are obstructed by an entropy bound violation, implying region-dependent interior reconstruction.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Almheiri, R. Mahajan, J. Maldacena, and Y. Zhao, \"The Page curve of Hawking radiation from semiclassical geometry,\"JHEP03(2020) 149, arXiv:1908.10996 [hep-th]. [4] A. Almheiri, N. Engelhardt, D. Marolf, and H. Maxfield, \"The entropy of bulk quantum fields and the entanglement wedge of an evaporating black hole,\" JHEP12(2019) 063,arXiv:1905.08762 [hep-th]. [5] A. Almheiri, R. Mahajan, and J. Maldacena, \"Islands outside the horizon,\"arXiv:1910.11077 [hep-th]. [6] A. Almheiri, T. Hartman, J. Maldacena, E. Shaghoulian, and A. Tajdini, \"The entropy of Hawking radiation,\"Rev. Mod. Phys.93no. 3, (2021) 035002,arXiv:2006.06872 [hep-th]. [7] M.-H. Yu and X.-H. Ge, \"Entanglement islands in generalized two-dimensional dilaton black holes,\"Phys."},{"citing_arxiv_id":"2604.11897","ref_index":199,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Particle detector in a position-superposed black hole spacetime","primary_cat":"quant-ph","submitted_at":"2026-04-13T18:00:08+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"An Unruh-DeWitt detector interacting with a position-superposed BTZ black hole produces outcome probabilities containing a nonclassical contribution that distinguishes quantum superposition from classical mixtures, arising from singularities in the probed spectrum.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Sandor, Quantum extremal islands made easy, part I: Entanglement on the brane (2020), arXiv:2006.04851 [hep-th]. [197] H. Z. Chen, R. C. Myers, D. Neuenfeld, I. A. Reyes, and J. Sandor, Quantum extremal islands made easy, part II: Black holes on the brane (2020), arXiv:2010.00018 [hep-th]. [198] R. Bousso and G. Penington, Islands far outside the horizon (2023), arXiv:2312.03078 [hep-th]. [199] A. Almheiri, R. Mahajan, and J. Maldacena, Islands outside the horizon (2019), arXiv:1910.11077 [hep-th]. [200] C. Krishnan, Critical islands, J. High Energy Phys.2021, 179. [201] M. V. Raamsdonk, Comments on wormholes, ensembles, and cosmology, J. High Energy Phys.2021, 156. [202] H. Geng, A. Karch, C. Perez-Pardavila, S. Raju, L. Ran- dall, M. Riojas, and S."},{"citing_arxiv_id":"2604.05815","ref_index":11,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Probing the Factorized Island Branch with the Capacity of Entanglement in JT Gravity","primary_cat":"hep-th","submitted_at":"2026-04-07T12:49:52+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"In JT gravity, the capacity of entanglement detects finite-n structure in the factorized island saddle that the entropy misses at first nontrivial order.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Penington,Entanglement wedge reconstruction and the information paradox, JHEP09 (2020) 002, arXiv:1905.08255. [9] G. Penington, S. H. Shenker, D. Stanford and Z. Yang,Replica wormholes and the black hole interior, JHEP03(2022) 205, arXiv:1911.11977. [10] A. Almheiri, T. Hartman, J. Maldacena, E. Shaghoulian and A. Tajdini,The entropy of Hawking radiation, Rev. Mod. Phys.93(2021) 035002, arXiv:2006.06872. [11] A. Almheiri, R. Mahajan and J. Maldacena,Islands outside the horizon, arXiv:1910.11077. [12] Y. Nakaguchi and T. Nishioka,A holographic proof of R' enyi entropic inequalities, JHEP12 (2016) 129, arXiv:1606.08443. [13] J. de Boer, J. J¨ arvel¨ a and E. Keski-Vakkuri,Aspects of capacity of entanglement, Phys. Rev. D99(2019) 066012, arXiv:1807.07357."},{"citing_arxiv_id":"2603.10102","ref_index":11,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Kerr Black Hole Ringdown in Effective Field Theory","primary_cat":"gr-qc","submitted_at":"2026-03-10T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Effective field theory yields model-independent corrections to Kerr black hole quasinormal modes that oscillate logarithmically near extremality, indicating discrete scale invariance.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2411.01105","ref_index":100,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"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":"[98] A. Almheiri, N. Engelhardt, D. Marolf and H. Maxfield,The entropy of bulk quantum fields and the entanglement wedge of an evaporating black hole, JHEP 12 (2019) 063 [arXiv:1905.08762]. [99] A. Almheiri, R. Mahajan, J. Maldacena and Y. Zhao,The Page curve of Hawking radiation from semiclassical geometry, JHEP 03 (2020) 149 [arXiv:1908.10996]. [100] A. Almheiri, R. Mahajan and J. Maldacena,Islands outside the horizon, arXiv:1910.11077. [101] G. Penington, S.H. Shenker, D. Stanford and Z. Yang,Replica wormholes and the black hole interior, JHEP 03 (2022) 205 [arXiv:1911.11977]. [102] A. Almheiri, T. Hartman, J. Maldacena, E. Shaghoulian and A. Tajdini,Replica Wormholes and the Entropy of Hawking Radiation, JHEP 05 (2020) 013 [arXiv:1911."},{"citing_arxiv_id":"1911.12333","ref_index":14,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Replica Wormholes and the Entropy of Hawking Radiation","primary_cat":"hep-th","submitted_at":"2019-11-27T18:23:34+00:00","verdict":"ACCEPT","verdict_confidence":"HIGH","novelty_score":8.0,"formal_verification":"none","one_line_summary":"Replica wormholes in the gravitational path integral yield the island rule for the fine-grained entropy of Hawking radiation, ensuring it follows the unitary Page curve in two-dimensional dilaton gravity.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"1911.11977","ref_index":18,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"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":"1905.08255","ref_index":87,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Entanglement Wedge Reconstruction and the Information Paradox","primary_cat":"hep-th","submitted_at":"2019-05-20T18:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":8.0,"formal_verification":"none","one_line_summary":"A phase transition in the quantum RT surface at the Page time derives the Page curve and enables entanglement wedge reconstruction of the black hole interior from Hawking radiation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}