{"total":12,"items":[{"citing_arxiv_id":"2605.28917","ref_index":68,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Greybody Factors, Absorption Cross Sections and Hawking Radiation of Holonomy-Corrected Schwarzschild Black Holes","primary_cat":"gr-qc","submitted_at":"2026-05-27T17:57:30+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Numerical study of holonomy-corrected Schwarzschild black holes finds enhanced low-frequency scalar transmission but overall suppressed Hawking radiation, with electromagnetic channel most quenched.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.25076","ref_index":85,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Grey-Body Factors and Thermodynamics of Asymptotically de Sitter Black Holes in Generalized Proca Theory","primary_cat":"gr-qc","submitted_at":"2026-05-24T13:39:39+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Applies sixth-order WKB to compute grey-body factors for test fields on generalized Proca black holes with effective de Sitter scale, finding that scalar mass and couplings raise barriers, suppress low-frequency transmission, and affect thermodynamics.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.21533","ref_index":71,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Long-lived quasinormal modes of Asymptotically de Sitter Black Holes in Generalized Proca Theory","primary_cat":"gr-qc","submitted_at":"2026-05-19T22:29:19+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Massive scalar perturbations of de Sitter black holes in generalized Proca theory enter a large-mass regime with linearly growing real frequencies and constant damping rates, without true quasi-resonances, plus an analytic formula and shifts due to black-hole size and Proca hair.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Opała, Phys. Rev. D 96, 024011 (2017), arXiv:1704.00361 [gr-qc]. [68] J. Matyjasek, R. A. Konoplya, and A. Zhidenko, Int. J. Grav. Theor. Phys. 2, 5 (2026), arXiv:2603.12466 [gr- qc]. [69] R. A. Konoplya and A. Zhidenko, Phys. Lett. B 686, 199 (2010), arXiv:0909.2138 [hep-th]. [70] Z. Malik, Int. J. Grav. Theor. Phys. 2, 3 (2026), arXiv:2603.18887 [gr-qc]. [71] S. V. Bolokhov and M. Skvortsova, Eur. Phys. J. C 86, 374 (2026), arXiv:2508.19989 [gr-qc]. [72] D. S. Eniceicu and M. Reece, Phys. Rev. D 102, 044015 (2020), arXiv:1912.05553 [gr-qc]. [73] S. Fernando, Gen. Rel. Grav. 48, 24 (2016), arXiv:1601.06407 [gr-qc]. [74] Y. Guo and Y.-G. Miao, Phys. Rev. D 102, 064049 (2020), arXiv:2005.07524 [hep-th]. [75] A."},{"citing_arxiv_id":"2605.12113","ref_index":45,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Quasinormal Spectra of Fields of Various Spin in Asymptotically de Sitter Black Holes within Generalized Proca Theory","primary_cat":"gr-qc","submitted_at":"2026-05-12T13:29:10+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Quasinormal frequencies for massless fields in Proca-hairy de Sitter black holes show scalar ℓ=0 modes most sensitive to hair parameter Q, with damping weakening near the three-horizon regime.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Opała, Phys. Rev. D 96, 024011 (2017), arXiv:1704.00361 [gr-qc]. [42] J. Matyjasek and M. Telecka, Phys. Rev. D 100, 124006 (2019), arXiv:1908.09389 [gr-qc]. [43] J. Matyjasek, R. A. Konoplya, and A. Zhidenko, Int. J. Grav. Theor. 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Phys. 2, 2 (2026),"},{"citing_arxiv_id":"2605.11364","ref_index":81,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Bardeen spacetime as quantum corrected black hole: Grey-body factors and quasinormal modes of gravitational perturbations","primary_cat":"gr-qc","submitted_at":"2026-05-12T00:34:59+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Increasing the quantum-correction scale in Bardeen spacetime raises quasinormal frequencies, slows decay, suppresses low-frequency transmission, and reorganizes absorption cross-sections.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"J. Mod. Phys. D 26, 1750112 (2017), arXiv:1703.10070 [gr-qc]. [78] Y. Guo and Y.-G. Miao, Phys. Rev. D 102, 064049 (2020), arXiv:2005.07524 [hep-th]. [79] R. A. Konoplya and A. Zhidenko, Phys. Lett. B 686, 199 (2010), arXiv:0909.2138 [hep-th]. [80] S. V. 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Skvortsova, Eur."},{"citing_arxiv_id":"2605.11013","ref_index":122,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Massive Scalar Quasinormal Modes, Greybody Factors, and Absorption Cross Section of a Parity-Symmetric Beyond-Horndeski Black Hole","primary_cat":"gr-qc","submitted_at":"2026-05-10T12:56:40+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Increasing the mass of a scalar field around a parity-symmetric beyond-Horndeski black hole strongly reduces the damping rate of quasinormal modes while suppressing low-frequency absorption and shifting efficient absorption to higher frequencies.","context_count":1,"top_context_role":"background","top_context_polarity":"unclear","context_text":"Zhidenko, JCAP 09, 068 (2024), arXiv:2406.11694 [gr-qc]. [119] R. A. Konoplya and A. Zhidenko, Phys. Lett. B 861, 139288 (2025), arXiv:2408.11162 [gr-qc]. [120] Z. 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Phys. 1, 4 (2025),"},{"citing_arxiv_id":"2605.03659","ref_index":63,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Long-lived massive scalar modes, grey-body factors, and absorption cross sections of the Reissner--Nordstr\\\"om-like brane-world black hole","primary_cat":"gr-qc","submitted_at":"2026-05-05T11:41:14+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Positive tidal charge in this brane-world black hole lowers the effective potential barrier, pushes massive scalar quasinormal modes toward arbitrarily long lifetimes, and increases transmission and absorption.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"D 102, 064049 (2020), arXiv:2005.07524 [hep-th]. [60] S. V. Bolokhov, K. A. Bronnikov, and M. V. Skvortsova, Int. J. Grav. Theor. Phys. 2, 2 (2026), arXiv:2507.14603 [gr-qc]. [61] R. A. Konoplya and A. Zhidenko, Phys. 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C 86,"},{"citing_arxiv_id":"2605.03137","ref_index":64,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Scattering of scalar, electromagnetic, and Dirac fields in an asymptotically flat regular black hole supported by primordial dark matter","primary_cat":"gr-qc","submitted_at":"2026-05-04T20:22:29+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Raising the regularity parameter in this regular black-hole spacetime lowers the single-barrier potentials for all three fields, shifts transmission to lower frequencies, increases absorption cross sections, and produces grey-body factors that agree with lowest-mode QNM reconstructions to roughly 10","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Zhidenko, Phys. Rev. D 82, 084003 (2010), arXiv:1004.3772 [hep-th]. [61] Z. Malik, Int. J. Grav. Theor. 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Bolokhov and M."},{"citing_arxiv_id":"2604.25471","ref_index":139,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Massive scalar quasinormal modes of an asymptotically flat regular black hole supported by a phantom Dirac--Born--Infeld field","primary_cat":"gr-qc","submitted_at":"2026-04-28T10:23:30+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Massive scalar quasinormal modes in this DBI-supported regular black hole show higher oscillation frequencies and lower damping as field mass increases, with larger regularity scales producing softer and longer-lived ringing.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.24349","ref_index":83,"ref_count":4,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter","primary_cat":"gr-qc","submitted_at":"2026-04-27T11:44:41+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Larger DBI regularity in this regular black hole model reduces quasinormal frequencies and damping rates for scalar, electromagnetic, and Dirac perturbations while the quality factor stays nearly constant, producing a robust spin-dependent ringdown signature.","context_count":2,"top_context_role":"background","top_context_polarity":"background","context_text":"[79] R. 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Bolokhov and M."},{"citing_arxiv_id":"2603.10844","ref_index":191,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Long-lived quasinormal modes, shadows and particle motion in four-dimensional quasi-topological gravity","primary_cat":"gr-qc","submitted_at":"2026-03-11T14:52:37+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Massive scalar quasinormal modes in quasi-topological black holes become long-lived as scalar mass grows, while photon-sphere radius, shadow size, and ISCO exhibit moderate deviations from Schwarzschild.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}