{"total":14,"items":[{"citing_arxiv_id":"2606.08631","ref_index":41,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Hawking Radiation from the Dymnikova Regular Black Hole","primary_cat":"gr-qc","submitted_at":"2026-06-07T13:50:43+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Numerical greybody factors for the Dymnikova black hole show temperature-driven luminosity suppression near the extremal remnant, with increasing fermion dominance in the residual massless flux.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.25705","ref_index":30,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Ces\\`aro convergence of the high-order WKB method and its applications to black-hole overtones and long-lived modes","primary_cat":"gr-qc","submitted_at":"2026-05-25T11:03:23+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"High-order WKB with Padé approximants and Cesàro means enables computation of black-hole overtones and long-lived quasinormal modes, with a noted limitation that apparent convergence can be incorrect for some metrics.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.25076","ref_index":67,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"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":85,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"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":"B 813, 136028 (2021), arXiv:1807.01792 [hep-th]. 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Zinhailo, EPL 149, 69004"},{"citing_arxiv_id":"2605.12113","ref_index":62,"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":"Zhidenko, Phys. Rev. D 83, 024031 (2011), arXiv:1011.1843 [gr- qc]. [59] Z. Malik, Int. J. Grav. Theor. Phys. 2, 3 (2026), arXiv:2603.18887 [gr-qc]. [60] M. Momennia, S. Hossein Hendi, and F. Soltani Bidgoli, Phys. Lett. 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Phys. 65, 45 (2026), arXiv:2511.00778 [gr-qc]."},{"citing_arxiv_id":"2605.03137","ref_index":84,"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":"Abdalla, Phys. Rev. D 71, 084015 (2005), arXiv:hep-th/0503029. [81] S. V. Bolokhov and M. Skvortsova, Eur. Phys. J. C 86, 374 (2026), arXiv:2508.19989 [gr-qc]. [82] B. C. Lütfüoğlu, Eur. Phys. J. C 85, 630 (2025), arXiv:2504.18482 [gr-qc]. [83] B. C. Lütfüoğlu, J. Rayimbaev, S. Murodov, J. Kur- banov, and M. Matyoqubov, (2026), arXiv:2604.14999 [gr-qc]. [84] B. C. Lütfüoğlu, Eur. Phys. J. C 86, 39 (2026), arXiv:2505.06966 [gr-qc]. [85] B. C. Lütfüoğlu, (2026), arXiv:2603.10844 [gr-qc]. [86] Z. Malik, Grav. Cosmol. 32, 122 (2026). [87] Z. Malik, Int. J. Theor. Phys. 63, 128 (2024), arXiv:2409.09872 [gr-qc]. [88] R. A. Konoplya and T. D. Pappas, JCAP 02, 038 (2026), arXiv:2507.01954 [gr-qc]. [89] Z. Malik, (2024), arXiv:2412."},{"citing_arxiv_id":"2604.26166","ref_index":55,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Scattering of electromagnetic field in quasi-topological gravity","primary_cat":"gr-qc","submitted_at":"2026-04-28T23:17:26+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Regular black holes in quasi-topological gravity produce shifted electromagnetic absorption spectra and modified photon sphere radii relative to singular Tangherlini solutions, with deviations suppressed as spacetime dimensions increase.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"L¨ utf¨ uo˘ glu, Long-lived quasinormal modes, grey-body factors and absorption cross-section of the black hole immersed in the Hernquist galactic halo, Phys. Lett. B872(2026) 140082 [2510.25969]. [54] Z. Malik, Correspondence between quasinormal modes and grey-body factors for massive fields in Schwarzschild-de Sitter spacetime, JCAP04(2025) 042 [2412.19443]. [55] B.C. L¨ utf¨ uo˘ glu, Quasinormal modes and gray-body factors for gravitational perturbations in asymptotically safe gravity, Eur. Phys. J. C86(2026) 39 [2505.06966]. [56] R.A. Konoplya and A. Zhidenko, Analytic expressions for quasinormal modes and grey-body factors in the eikonal limit and beyond, Class. Quant. Grav.40(2023) 245005 [2309.02560]."},{"citing_arxiv_id":"2603.10844","ref_index":170,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"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},{"citing_arxiv_id":"2601.22340","ref_index":110,"ref_count":2,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Grey-body factors of higher dimensional regular black holes in quasi-topological theories","primary_cat":"gr-qc","submitted_at":"2026-01-29T21:33:15+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Higher dimensional regular black holes in quasi-topological gravity have suppressed grey-body factors and Hawking radiation compared to singular black holes in general relativity.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2601.18613","ref_index":56,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Correspondence between quasinormal modes and grey-body factors of Schwarzschild--Tangherlini black holes","primary_cat":"gr-qc","submitted_at":"2026-01-26T15:53:33+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Quasinormal modes correspond well to grey-body factors for vector and tensor perturbations of Schwarzschild-Tangherlini black holes in all dimensions, but fail for scalar l=2 modes in D≥7 because of multiple potential barriers.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2512.23510","ref_index":28,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Quasinormal mode/grey-body factor correspondence for Kerr black holes","primary_cat":"gr-qc","submitted_at":"2025-12-29T14:47:19+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"WKB analysis of the Teukolsky equation establishes a quasinormal-mode to greybody-factor correspondence for Kerr black holes that holds in the eikonal limit for gravitational perturbations and matches numerics at high angular momentum.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2506.16217","ref_index":75,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Quasinormal modes and grey-body factors of axial gravitational perturbations of regular black holes in asymptotically safe gravity","primary_cat":"gr-qc","submitted_at":"2025-06-19T11:09:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Axial quasinormal modes of regular black holes in asymptotically safe gravity are weakly affected by the deviation parameter for the fundamental mode but show notable deviations for higher overtones, with strong agreement between grey-body factors and QNMs for large multipole numbers.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}