{"total":10,"items":[{"citing_arxiv_id":"2606.30507","ref_index":133,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"The Role of the Volume in Black Hole Thermodynamics","primary_cat":"gr-qc","submitted_at":"2026-06-29T16:13:54+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Conserved charges built from a Kerr-Schild background show the first law requires the Killing vector and AdS background to be held fixed, explaining why the rotating-frame energy F fails while E works, and why the geometric volume appears in the β Smarr relation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.28427","ref_index":7,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Reverse Isoperimetric Conjecture as a Noether-Charge Stability Theorem","primary_cat":"gr-qc","submitted_at":"2026-06-25T20:09:09+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"The reverse isoperimetric conjecture is proven to be the fixed-volume form of a boundary-completed Noether-charge stability theorem.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.26163","ref_index":28,"ref_count":2,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Large-$N$ Carrollian Thermodynamics from AdS Black-Hole Phase-Space Contractions","primary_cat":"hep-th","submitted_at":"2026-06-24T06:24:41+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Finite Carrollian black-hole thermodynamics arises as a double-scaled low-temperature large-N ensemble in AdS/CFT, with the boundary Brown-York stress tensor reproducing the contracted bulk Hamiltonian and first law.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.09443","ref_index":71,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Perturbative study of Supercritical Crossover in Noncommutative-corrected Spacetime","primary_cat":"hep-th","submitted_at":"2026-06-08T12:51:35+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Noncommutative corrections preserve the mean-field universality class of the supercritical crossover and Widom line in charged AdS black holes.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.24091","ref_index":13,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Hawking atmosphere of anti-de Sitter black holes","primary_cat":"gr-qc","submitted_at":"2026-05-22T18:00:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Applies Parikh-Wilczek tunneling with backreaction to evaporating AdS black holes, finding luminosity deviates from blackbody scaling for small masses due to rapid mass loss, and computes renormalized energy-momentum tensor in Vaidya-AdS.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.22429","ref_index":57,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Black Hole Entropy Beyond the Wald Term in Nonminimally Coupled Gravity: A Covariant Phase Space Decomposition","primary_cat":"gr-qc","submitted_at":"2026-05-21T12:51:49+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Black hole entropy in diffeomorphism-invariant nonminimal gravity decomposes as S_H = S_W + S_1 + ΔS, with the extra terms required for bumblebee and Weyl-vector Gauss-Bonnet solutions but not for regular Kalb-Ramond branches.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.16536","ref_index":25,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Quantum-statistical constraints on Kerr-anti-de Sitter thermodynamics","primary_cat":"gr-qc","submitted_at":"2026-05-15T18:32:30+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Quantum-statistical constraints restrict the infinite family of KadS thermodynamic descriptions to a subclass that reduces to Schwarzschild-AdS and Kerr cases in appropriate limits, with uniqueness for co-rotating and volume-coincident descriptions.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.03311","ref_index":47,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Noether charges and the first law of thermodynamics for multifractional Schwarzschild black hole in the q-derivative theory","primary_cat":"gr-qc","submitted_at":"2026-05-05T02:57:39+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Multi-fractional Schwarzschild black holes have profile-insensitive Noether mass and geometric area-law entropy, but require an extended first law with work terms for the q-profile parameters to restore integrability of the Clausius relation.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"A useful way to interpret presentation dependence, advocated in Ref. [ 30], is to regard the presentation as an effective parametrization of an underlying microscopic (possibly stochastic) structure. This perspective is consistent with the broader association between dimensional flow and an effectively stochastic spacetime fuzziness discussed in Ref. [ 47]. In that view one does not assign an operational preference to either sign in Eq. (VI.1), but instead treats the induced spread in fractional-frame observables as an intrinsic uncertainty band [ 30]. For any quantity O that depends on the profile choice, one may then define the presentation average and half-spread as ⟨O⟩± = O+ +O − 2 , ∆±O= |O+ − O−|"},{"citing_arxiv_id":"2601.00771","ref_index":29,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Extremalization approach to black hole thermodynamics: perturbations around higher-derivative gravities","primary_cat":"gr-qc","submitted_at":"2026-01-02T18:06:47+00:00","verdict":"ACCEPT","verdict_confidence":"MODERATE","novelty_score":4.0,"formal_verification":"none","one_line_summary":"The Reall–Santos extremalization method is extended to perturbations around Einstein–Gauss–Bonnet backgrounds, reproducing known quasi-topological black-hole thermodynamics without solving the perturbed metric.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2512.01916","ref_index":7,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Explicit and covariant formula for thermodynamic volume in extended black hole thermodynamics","primary_cat":"gr-qc","submitted_at":"2025-12-01T17:33:08+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"An explicit covariant formula for thermodynamic volume is derived that universally decomposes into explicit Lagrangian coupling dependence plus dynamical field response contributions.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}