{"total":12,"items":[{"citing_arxiv_id":"2606.31705","ref_index":51,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Monitoring a de Sitter universe through an anti-de Sitter window","primary_cat":"hep-th","submitted_at":"2026-06-30T14:11:52+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Proposes a duality between AdS3 gravity with dS2 branes and CFT2 with non-unitary boundary conditions to realize dS holography via complex saddles and state preparation in unitary AdS/CFT.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.21079","ref_index":11,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Linear Growth of Holographic Time-like Entanglement Entropy and Kasner exponents","primary_cat":"hep-th","submitted_at":"2026-06-19T03:59:53+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"In asymptotically AdS black holes with space-like singularities, late-time linear growth of time-like entanglement entropy is governed by a critical extremal surface inside the event horizon, with growth rates bounded by Kasner exponents under null and dominant energy conditions.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.20790","ref_index":55,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Complexity Inequalities for Quantum Subsystems","primary_cat":"hep-th","submitted_at":"2026-06-18T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Defines tripartite complexity and complexity gap for three-subsystem states and reports that the gap has definite sign across holographic CV, Fisher-Rao, and Krylov measures, suggesting it as a building block for complexity inequalities.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.03977","ref_index":31,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Pure states for subregions in gravity and their entanglement entropy","primary_cat":"hep-th","submitted_at":"2026-06-02T17:56:33+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A construction assigns pure states to subregions in quantum gravity via partially frozen path integrals and gives a holographic prescription for their entanglement entropy that satisfies consistency conditions and recovers known formulas.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.01296","ref_index":13,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Notes on Wasserstein distance and wormholes","primary_cat":"hep-th","submitted_at":"2026-05-31T15:33:47+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Defines Boltzmann-Wasserstein distance on quantum theories via optimal W2 transport of Boltzmann-weighted spectra, equates it to thermal correlators, and constructs a Schwinger-Keldysh wormhole saddle that reproduces the spectral optimum.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.00488","ref_index":24,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Massless Islands in Wedge Holography","primary_cat":"hep-th","submitted_at":"2026-05-30T02:39:47+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"A unitary defect CFT at the wedge corner supplies an auxiliary holographic entropy term that balances area variations and enables stable non-horizon islands in massless ghost-free wedge holography.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.23670","ref_index":42,"ref_count":2,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Twirled Perfect Tensor Networks: Computationally covariant holographic tensor networks","primary_cat":"hep-th","submitted_at":"2026-05-22T14:18:32+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Twirled perfect tensor networks achieve computational covariance, bound complexity by the PLC, and obey a lattice Ryu-Takayanagi formula for arbitrary boundary subregions.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.02514","ref_index":46,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Holographic Banners","primary_cat":"hep-th","submitted_at":"2026-04-02T21:16:13+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":8.0,"formal_verification":"none","one_line_summary":"Holographic banners are four-argument on-shell actions that map thermofield double boundary states to future interior semiclassical states and yield BKL mixing timescales in AdS black holes.","context_count":1,"top_context_role":"background","top_context_polarity":"support","context_text":"interior, JHEP07, 202, 2024, [arXiv:2312.11622 [hep-th]]. 33 [43] M. De Clerck, An introduction to BKL theory, PoSModave2024, 002, 2026. [44] E. B. Bogomolny, B. Georgeot, M. J. Giannoni and C. Schmit, Arithmetical chaos, Phys. Rept.291, 219-324, 1997. [45] J. Marklof, Arithmetic quantum chaos, inEncyclopedia of Mathematical Physics, Vol 1, pp. 212-220. Amsterdam: Elsevier, 2004. [46] T. Hartman and J. Maldacena, Time Evolution of Entanglement Entropy from Black Hole Interiors, JHEP05, 014, 2013, [arXiv:1303.1080 [hep-th]]. [47] S. H. Shenker and D. Stanford, Black holes and the butterfly effect, JHEP03, 067, 2014, [arXiv:1306.0622 [hep-th]]. [48] L. Susskind, Computational Complexity and Black Hole Horizons, Fortsch. Phys.64,"},{"citing_arxiv_id":"2507.06286","ref_index":159,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Krylov Complexity","primary_cat":"hep-th","submitted_at":"2025-07-08T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"Krylov complexity is a canonical, parameter-independent measure of operator spreading that probes chaotic dynamics to late times and admits a geometric interpretation in holographic duals.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2412.18610","ref_index":14,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Crosscap Quenches and Entanglement Evolution","primary_cat":"hep-th","submitted_at":"2024-12-24T18:59:58+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Introduces crosscap quenches in CFTs and holographic models to derive universal entanglement entropy evolution, validated by numerics in spin systems.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"1911.12333","ref_index":62,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"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":"1908.10996","ref_index":42,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The Page curve of Hawking radiation from semiclassical geometry","primary_cat":"hep-th","submitted_at":"2019-08-29T00:37:46+00:00","verdict":"ACCEPT","verdict_confidence":"MODERATE","novelty_score":8.0,"formal_verification":"none","one_line_summary":"Hawking radiation entropy follows the Page curve when quantum extremal surfaces are identified with RT/HRT surfaces in a higher-dimensional holographic dual, making the black hole interior part of the radiation's entanglement wedge.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}