{"total":17,"items":[{"citing_arxiv_id":"2606.30818","ref_index":31,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Black holes in a bouncing universe","primary_cat":"gr-qc","submitted_at":"2026-06-29T18:45:06+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Two-fluid model shows black holes persist through cosmological bounce and modify background fluid properties under fixed geometry.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.30233","ref_index":3,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Complex Phase Structure and Widom line for Euler Heisenberg black holes","primary_cat":"hep-th","submitted_at":"2026-06-29T12:45:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Euler-Heisenberg AdS black holes show a four-phase structure with two critical points and multiple Widom lines in the complex plane under Lee-Yang analysis.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.20314","ref_index":1,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Macroscopic Black-Hole Remnants in a Nonlocal Field Theory: Towards Hawking Radiation in SFT","primary_cat":"hep-th","submitted_at":"2026-06-18T14:48:08+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"In a smeared massless scalar on dynamical black hole, outgoing particle number drops to zero after scrambling time due to SFT nonlocality, implying macroscopic remnant.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.19110","ref_index":30,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Kiselev black hole and the ultra-slow evaporating behavior","primary_cat":"gr-qc","submitted_at":"2026-06-17T14:23:45+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Lowering the quintessence state parameter w_q in Kiselev black holes produces ultra-slow evaporation distinct from PFDM and Horndeski cases, offering a possible constraint on w_q.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.13539","ref_index":4,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Conformally Invariant Corrections to the Anomaly-Induced Effective Action and Black Hole Evaporation in Four Dimensions","primary_cat":"hep-th","submitted_at":"2026-06-11T16:23:37+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Conformally invariant corrections to the anomaly-induced effective action produce a one-parameter family of quantum hair for Schwarzschild black holes that modifies the near-horizon stress tensor in a static approximation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.03316","ref_index":4,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Possible explanation of primordial $^7$Li deficit","primary_cat":"astro-ph.CO","submitted_at":"2026-06-02T08:27:44+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Baryons from evaporating primordial black holes reduce primordial ^7Li abundance to observed values via neutron capture converting it to ^4He.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.26372","ref_index":66,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Thermodynamics and quasinormal modes of the regular Dymnikova-Letelier black hole","primary_cat":"gr-qc","submitted_at":"2026-05-25T22:42:03+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"Thermodynamic analysis of the Dymnikova-Letelier regular black hole reveals string-fluid-dependent phase transitions, while sixth-order WKB shows stable scalar quasinormal modes with shifted frequencies and damping rates.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.25497","ref_index":2,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Degenerate Bifurcations and Universal Relaxation Scaling in Black Hole Thermodynamics","primary_cat":"hep-th","submitted_at":"2026-05-25T06:57:27+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Black hole thermodynamic criticality exhibits universal relaxation scaling and critical slowing down determined by local bifurcation structures.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.15655","ref_index":3,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Critical slowing down of black hole phase transition and universal dynamic scaling in AdS black holes","primary_cat":"hep-th","submitted_at":"2026-05-15T06:24:27+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Black hole phase transitions in AdS spacetime show critical slowing down with relaxation time scaling as τ = |ε|^{-2/3}, and this exponent is the same for RN-AdS, Kerr-AdS, and Bardeen black holes.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.10476","ref_index":84,"ref_count":2,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Breaking Free from the Swampland of Impossible Universes through the DESI Portal","primary_cat":"astro-ph.CO","submitted_at":"2026-05-11T12:38:17+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"A review summarizing advancements over the past two years that link DESI baryon acoustic oscillation data to string-inspired scenarios with dynamic dark energy.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"3847/1538-4357/ae4738 [arXiv:2512.07281 [astro-ph.CO]]. [82] R. R. Caldwell, M. Kamionkowski and N. N. Weinberg, Phantom energy and cosmic dooms- day, Phys. Rev. Lett.91, 071301 (2003) doi:10.1103/PhysRevLett.91.071301 [arXiv:astro- ph/0302506 [astro-ph]]. [83] J. D. Bekenstein, Black holes and entropy, Phys. Rev. D7, 2333-2346 (1973) doi:10.1103/PhysRevD.7.2333 [84] S. W. Hawking, Black hole explosions, Nature248, 30-31 (1974) doi:10.1038/248030a0 [85] C. Vafa, Swamplandish Unification of the Dark Sector, [arXiv:2402.00981 [hep-ph]]. [86] T. Kaluza, Zum Unit¨ atsproblem der Physik, Sitzungsber. Preuss. Akad. Wiss. Berlin (Math. Phys.)1921, 966-972 (1921) doi:10.1142/S0218271818700017 [arXiv:1803.08616 [physics."},{"citing_arxiv_id":"2605.00780","ref_index":5,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Breakdown of Semiclassical Gravity in Four-Dimensional Black Hole Evaporation","primary_cat":"hep-th","submitted_at":"2026-05-01T16:54:38+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Semiclassical black hole evaporation in four dimensions produces a thunderbolt singularity signaling breakdown of the effective theory at large distances.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Much of this intuition about semiclassical black hole evap- oration has been shaped by lower-dimensional toy models, most notably two-dimensional dilaton gravity, where calculations are tractable and explicit analytic results can be ob- tained [2-4]. The situation is less clear in four spacetime dimensions. While Hawking's original calculation demonstrated that black holes radiate [5, 6], incorporating the back- reaction of this radiation on the spacetime geometry has proven technically challenging. The nonlocal structure of the effective action induced by quantum matter fields, together with the complexity of the four-dimensional semiclassical Einstein equations, has held back progress toward a definitive description of four-dimensional black hole evaporation."},{"citing_arxiv_id":"2604.25495","ref_index":4,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Phase Transitions and Chaos Bound in Horava Lifshitz Black Holes using Lyapunov Exponents","primary_cat":"hep-th","submitted_at":"2026-04-28T10:55:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Lyapunov exponents act as order parameters for first-order phase transitions in Horava-Lifshitz black holes with mean-field critical exponent 1/2, while chaos bounds are violated below a horizon-radius threshold even in stable phases.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"deeply connected. [1] S. W. Hawking, \"Gravitational radiation from colliding black holes,\" Phys. Rev. Lett.26, 1344-1346 (1971) doi:10.1103/PhysRevLett.26.1344 [2] J. Bekenstein, \"Bekenstein-Hawking entropy,\" Scholarpedia3, no.10, 7375 (2008) doi:10.4249/scholarpedia.7375 [3] S. W. Hawking, \"Black hole explosions,\" Nature248, 30-31 (1974) doi:10.1038/248030a0 [4] S. W. Hawking, \"Particle Creation by Black Holes,\" Commun. Math. Phys.43, 199-220 (1975) [erratum: Commun. Math. Phys.46, 206 (1976)] doi:10.1007/BF02345020 [5] J. M. Bardeen, B. Carter and S. W. Hawking, \"The Four laws of black hole mechanics,\" Commun. Math. Phys.31, 161-170 (1973) doi:10.1007/BF01645742 [6] P. C. W. Davies, \"Thermodynamics of Black Holes,\" Proc."},{"citing_arxiv_id":"2604.17017","ref_index":105,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Transiently accelerating cosmological model with Gong-Zhang parametrization in $f(T)$ teleparallel gravity","primary_cat":"gr-qc","submitted_at":"2026-04-18T14:56:30+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"In f(T) gravity with Gong-Zhang EoS parametrization, the fitted model shows transient acceleration followed by future deceleration and satisfies thermodynamic consistency.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"fluid inside the horizon, ( Tin) is equal to the temperature of the dynamical apparent horiz on ( Th) [104]. This temperature is identified with the Hayward-Kodama temperat ure and can be expressed as Th = 2H 2 + ˙H 4π H . (43) It is worth noting that, in the de Sitter spacetime where ˙H = 0, this temperature reduces to the Hawking temperature, THawking = H 2π [105]. By employing Eqs. (42) and (43), we obtain the rate of c hange of entropy of the fluid enclosed within the horizon as ˙Sin = 16π 2 ˙H H 3 ( 1 + ˙H 2H 2 + ˙H ) . (44) Using Eqs. (38), (40) and (44), we derive the expression for t he rate of change of the total entropy as ˙Stot = ( 4π ˙H H2 ) 2 H ( ˙H H2 + 2 ) . (45) The validity of the GSLT requires that the time derivative of the total entropy satisfies ˙Stot ≥ 0; otherwise,"},{"citing_arxiv_id":"2604.04695","ref_index":68,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"EHT-Constrained Analysis of Shadow Deformation in Quantum-Improved Rotating Non-Singular Magnetic Monopole","primary_cat":"gr-qc","submitted_at":"2026-04-06T14:03:46+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"Increasing the asymptotic safety parameter and spin shrinks the shadow size while increasing its distortion for a rotating Bardeen black hole, with monopole charge shaping the profile and energy emission rates also computed.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Phys. 6 (1965) 915-917, doi:10.1063/1.1704350. [66] M. Azreg-A¨ ınou, \"Generating rotating regular black hole s o- lutions without complexification,\" Phys. Rev. D 90, 064041 (2014), arXiv:1405.2569 [gr-qc]. [67] B. Toshmatov, Z. Stuchl' ık, and B. Ahmedov, \"Rotating black hole solutions with quintessential energy,\" Eur . Phys. J. Plus 132, 98 (2017). [68] C. A. Benavides-Gallego, A. Abdujabbarov, and C. Bambi, \"Rotating and nonlinear magnetic-charged black hole sur- rounded by quintessence,\" Phys. Rev. D 101, 044038 (2020). [69] R. M. Wald, General Relativity (University of Chicago Press, Chicago, 2010). [70] C. Bambi and L. Modesto, \"Rotating regular black holes,\" Phys. Lett. B 721, 329-334 (2013)."},{"citing_arxiv_id":"2601.18422","ref_index":6,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Time-reversed Shannon entropy as a chaos indicator for non-integrable systems","primary_cat":"gr-qc","submitted_at":"2026-01-26T12:32:34+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Time-reversed Shannon entropy distinguishes chaotic from regular orbits in Kerr and Schwarzschild-Melvin spacetimes by quantifying forward-backward asymmetry in probability distributions.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2504.11205","ref_index":13,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Probing Black Hole Phase Transitions through Quasi-Periodic Oscillations","primary_cat":"gr-qc","submitted_at":"2025-04-15T14:07:49+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"QPO frequencies in RN AdS and Kerr geometries trace distinct thermodynamic phases and their stability when plotted against Hawking temperature.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2412.08337","ref_index":42,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Thermodynamic Behavior of a 4D Nonminimal Maxwell-AdS Black Hole","primary_cat":"hep-th","submitted_at":"2024-12-11T12:24:46+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Derives perturbative 4D nonminimal Maxwell-AdS black hole and reports Van der Waals-like behavior plus Hawking-Page transitions in its thermodynamics.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}