{"total":14,"items":[{"citing_arxiv_id":"2606.29899","ref_index":59,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Quantum (non)equivalence of dual massive $p$-form gauge theories","primary_cat":"hep-th","submitted_at":"2026-06-29T07:35:21+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Path integral quantization of topologically coupled massive p-form theories shows quantum duality breaking on non-trivial backgrounds, with the difference in required counterterms proportional to the Euler characteristic.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.22810","ref_index":35,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A Linearized Obstruction to the Supersymmetric Extension of Conformal Boundary Conditions in Euclidean Gravity","primary_cat":"hep-th","submitted_at":"2026-06-22T03:39:57+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Witten's conformal boundary condition admits no half-supersymmetric extension in linearized minimal supergravity because supersymmetry maps the natural gravitino datum to the trace-free extrinsic curvature left unfixed by the conformal prescription.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.17149","ref_index":7,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Extended Supergravity Needs String Scale Cut-off","primary_cat":"hep-th","submitted_at":"2026-06-15T18:00:03+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"String-scale UV cut-off in the gravitational path integral removes string-coupling dependence from the BPS black hole index in extended supergravity, matching supersymmetry expectations for zero-Euler-number cases.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.11984","ref_index":9,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Modular quantization and black holes","primary_cat":"hep-th","submitted_at":"2026-06-10T12:07:41+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Modular quantization of a single holographic CFT reproduces exact Hartle-Hawking correlators of smooth BTZ black holes in the semiclassical limit while yielding non-smooth stretched-horizon descriptions at finite GN.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"This line of reasoning subsequently led to the formulation of the 'firewall paradox'2 [7], [8]. In this fuzzball/firewall paradigm, the central theme is to replace the 'smooth' nature of semiclassical horizon to restore unitarity. Over the past decade, remarkable progress has been achieved through the study of Euclidean gravitational path integrals [9]- [16]. In particular, certain Euclidean wormhole saddles have played a central role in reproducing the Page curve via the quantum extremal surface (QES) prescription [17]. Despite their striking success, the precise physical origin and interpretation of these wormholes remain poorly understood within the Euclidean gravitational path integral framework itself3."},{"citing_arxiv_id":"2606.08047","ref_index":12,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Warped Product Einstein Manifolds in Four Dimensions","primary_cat":"gr-qc","submitted_at":"2026-06-06T08:20:56+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Einstein warped products in 4D are classified algebraically via curvature matrix blocks into Petrov types (3+1 generically type I, 2+2 type D, 1+3 type O), with closed Riemannian half-conformally flat cases required to be flat.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.30417","ref_index":24,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Logarithm of charge ratio in black hole entropy","primary_cat":"hep-th","submitted_at":"2026-05-28T18:00:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Macroscopic computation of charge-ratio logarithmic corrections to black hole entropy agrees with microscopic results in N=4 and N=8 string theories after including string-scale cutoff, dilaton-dependent measure, Kalb-Ramond variable, and microcanonical ensemble.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.14668","ref_index":82,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"$\\alpha'$ corrections to self-dual gravitational instantons","primary_cat":"hep-th","submitted_at":"2026-05-14T10:25:43+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"α' corrections leave the metric of self-dual instantons unmodified but correct the dilaton and axion fields via Gauss-Bonnet and Pontrjagin terms, with no net correction to the Euclidean action to first order.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.27046","ref_index":51,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Tidal Response and Thermodynamics of Black Holes","primary_cat":"hep-th","submitted_at":"2026-04-29T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A new gauge-invariant effective action computes black hole Love numbers without Regge-Wheeler methods, and these numbers determine leading thermodynamic corrections under external perturbations.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"festly gauge invariant, as it avoids introducing propagators for long-distance fields and thus eliminates the need for gauge fixing. The resulting Love numbers are in full agreement with known results, and the method can be readily extended to other types of perturbations. The second focus of this paper is the connection between Love numbers and black hole thermodynamics [51, 52]. The thermodynamic description of a black hole depends strongly on the asymptotic structure of spacetime [53, 54]. Assumptions about asymptotics determine how quantities such as energy, temperature, and entropy are defined, as well as the appropriate thermodynamic ensemble. While one typically assumes asymptotically flat, Anti-de Sitter, or de Sitter boundary conditions, such assumptions tend to obscure"},{"citing_arxiv_id":"2604.21736","ref_index":10,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"IR behaviour of one-loop complex $\\mathbb{R}\\times S^3$ saddles","primary_cat":"hep-th","submitted_at":"2026-04-23T14:40:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"One-loop metric fluctuations produce secularly growing IR divergences in the Hartle-Hawking wavefunction for complex saddles on R x S3, identical in leading order to the Lorentzian de Sitter case after UV renormalization.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"20(1974), 69-94 [8] S. Deser, H. S. Tsao and P. van Nieuwenhuizen, \"Nonrenormalizability of Einstein Yang-Mills Interactions at the One Loop Level,\" Phys. Lett. B50(1974), 491-493 doi:10.1016/0370- 2693(74)90268-8 [9] M. H. Goroff and A. Sagnotti, \"The Ultraviolet Behavior of Einstein Gravity,\" Nucl. Phys. B 266(1986), 709-736 doi:10.1016/0550-3213(86)90193-8 [10] A. Salam and J. A. Strathdee, \"Remarks on High-energy Stability and Renormalizability of Gravity Theory,\" Phys. Rev. D18(1978), 4480 doi:10.1103/PhysRevD.18.4480 [11] G. Narain and R. Anishetty, \"Short Distance Freedom of Quantum Gravity,\" Phys. Lett. B 711(2012), 128-131 doi:10.1016/j.physletb.2012.03.070 [arXiv:1109.3981 [hep-th]]. [12] L. P. Grishchuk, \"Amplification of gravitational waves in an isotropic universe,\" Sov."},{"citing_arxiv_id":"2604.21014","ref_index":34,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"3D near-de Sitter gravity and the soft mode of DSSYK","primary_cat":"hep-th","submitted_at":"2026-04-22T19:01:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"The soft mode of DSSYK is dual to 3D near-de Sitter gravity with a localized dS2 slice, where effective actions, entropies, and correlators match via conformal boundary conditions on future and past infinity.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"[32] Venkatesa Chandrasekaran, Roberto Longo, Geoff Penington, and Edward Witten. \"An algebra of observables for de Sitter space\". In:JHEP02 (2023), p. 082.doi:10.1007/JHEP02(2023)082. arXiv:2206.10780 [hep-th]. [33] G. W. Gibbons and S. W. Hawking. \"Action Integrals and Partition Functions in Quantum Gravity\". In:Phys. Rev. D15 (1977), pp. 2752-2756.doi:10.1103/PhysRevD.15.2752. [34] James W. York. \"Role of Conformal Three-Geometry in the Dynamics of Gravitation\". In:Phys. Rev. Lett.28 (16 Apr. 1972), pp. 1082-1085.doi:10.1103/PhysRevLett.28.1082.url:https: //link.aps.org/doi/10.1103/PhysRevLett.28.1082. [35] G. Hayward. \"Gravitational action for space-times with nonsmooth boundaries\". In:Phys. Rev. D47 (1993), pp. 3275-3280.doi:10."},{"citing_arxiv_id":"2604.19831","ref_index":22,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Van der Waals Gravity Theory","primary_cat":"gr-qc","submitted_at":"2026-04-20T22:56:32+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"A van der Waals-inspired modification to general relativity renders the gravitational coupling dynamical, providing a mechanism to avoid Big Bang and black hole singularities.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"1936 (2006) doi:10.1142/S021827180600942X [arXiv:hep-th/0603057 [hep-th]]. [20] A. G. Riesset al.[Supernova Search Team], Astron. J.116, 1009-1038 (1998) doi:10.1086/300499 [arXiv:astro-ph/9805201 [astro-ph]]. [21] S. Perlmutteret al.[Supernova Cosmology Project], Astrophys. J.517, 565-586 (1999) doi:10.1086/307221 [arXiv:astro-ph/9812133 [astro-ph]]. [22] G. W. Gibbons and S. W. Hawking, Phys. Rev. D15, 2752-2756 (1977) doi:10.1103/PhysRevD.15.2752 [23] B. S. DeWitt, Phys. Rev.162, 1239-1256 (1967) doi:10.1103/PhysRev.162.1239 [24] A. Ashtekar, J. Baez, A. Corichi and K. Kras- nov, Phys. Rev. Lett.80, 904-907 (1998) doi:10.1103/PhysRevLett.80.904 [arXiv:gr- qc/9710007 [gr-qc]]. [25] G. 't Hooft and M."},{"citing_arxiv_id":"2508.06725","ref_index":88,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Thermal and Optical Signatures of Einstein-Dyonic ModMax Black Holes with GUP and Plasma Modifications","primary_cat":"gr-qc","submitted_at":"2025-08-08T21:44:23+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"The paper derives GUP-modified Hawking radiation spectra and Gauss-Bonnet light deflection angles for Einstein-Dyonic-ModMax black holes in vacuum and plasma, along with quantum-corrected thermodynamics showing phase transitions.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Dark matter from axion strings with adaptive mesh refinement.Nature Commun., 13(1): 1049, 2022. doi: 10.1038/s41467-022-28669-y. [86] Georg Raffelt and Leo Stodolsky. Mixing of the Photon with Low Mass Particles.Phys. Rev. D , 37:1237, 1988. doi: 10.1103/PhysRevD.37.1237. [87] Peter Svrcek and Edward Witten. Axions In String Theory.JHEP, 06:051, 2006. doi: 10.1088/1126-6708/ 2006/06/051. [88] David J. E. Marsh. Axion Cosmology.Phys. Rept., 643:1-79, 2016. doi: 10.1016/j.physrep.2016.06.005. [89] Farruh Atamurotov, Kimet Jusufi, Mubasher Jamil, Ahmadjon Abdujabbarov, and Mustapha Azreg-Aïnou. Axion-plasmonormagnetizedplasmaeffectonanobservableshadowandgravitationallensingofaSchwarzschild black hole. Phys. Rev. D , 104(6):064053, 2021. doi: 10."},{"citing_arxiv_id":"2504.17081","ref_index":81,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A new rotating axionic AdS$_4$ black hole dressed with a scalar field","primary_cat":"hep-th","submitted_at":"2025-04-23T20:06:31+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"A new axionically charged rotating AdS4 black hole solution with scalar field is presented, defined by a structural function and parameters, with thermodynamics derived via Euclidean method satisfying the first law.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"with the field space metric given by ds2 = dϕ2 + ε(ϕ)dψ2. The associated scalar curvature R of this two-dimensional field space geometry reads R = − d dϕ \u0012 dε(ϕ)/dϕ ε(ϕ) \u0013 − 1 2 \u0012 dε(ϕ)/dϕ ε(ϕ) \u00132 , which, in general, is not constant. Unlike the typical situation in supergravity models, where scalar manifolds are often realized as symmetric coset spaces with constant curvature [81, 82], the geometry emerging in this case does not correspond to any standard maximally symmetric space or its non-compact counterparts [83]. This makes the existence of such a configuration particularly intriguing, suggesting a nontrivial interplay between the scalar sector and the underlying dynamics. Secondly, the inclusion of a rotational component offers"},{"citing_arxiv_id":"1907.03619","ref_index":27,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Gravity, Superselection Rules and Axions","primary_cat":"hep-th","submitted_at":"2019-07-08T13:59:18+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Quantum gravity forces the QCD theta parameter to emerge as the vev of a local axion field through coherent-state representations of geometry and a quantum-information interpretation of topological-charge superselection.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}