{"total":14,"items":[{"citing_arxiv_id":"2606.08631","ref_index":68,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"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":"2606.08351","ref_index":54,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Hawking Emission from Black Holes Evaporating toward Wormholes and the Accuracy of the WKB Approximation","primary_cat":"gr-qc","submitted_at":"2026-06-06T21:52:07+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Numerical greybody factors for photons and massless Dirac fields in Simpson-Visser and Casadio-Fabbri-Mazzacurati geometries reveal that WKB overestimates luminosities by orders of magnitude near wormhole endpoints, increasing a Simpson-Visser lifetime coefficient by a factor of about 85.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.03842","ref_index":49,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Scattering and Hawking Radiation from Einstein--Euler--Heisenberg--de Sitter Black Holes","primary_cat":"gr-qc","submitted_at":"2026-06-02T16:21:06+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Numerical scattering calculations for neutral scalar and Dirac fields on Einstein-Euler-Heisenberg-de Sitter black holes show that Euler-Heisenberg coupling raises barriers and shifts transmission frequencies upward while cosmological constant lowers thresholds, with luminosity highly sensitive to t","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.28917","ref_index":18,"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":48,"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":127,"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":"Malik, JCAP 04, 042 (2025), arXiv:2412.19443 [gr- qc]. [124] B. C. Lütfüoğlu, A. Shermatov, J. Rayimbaev, M. Maty- oqubov, and O. Sirajiddin, Eur. Phys. J. C 85, 1484 (2025), arXiv:2511.22366 [gr-qc]. [125] R. A. Konoplya and A. Zhidenko, Phys. Rev. D 82, 084003 (2010), arXiv:1004.3772 [hep-th]. [126] A. Dubinsky, Mod. Phys. Lett. A 40, 2550111 (2025), arXiv:2412.00625 [gr-qc]. [127] B. C. Lütfüoğlu, Int. J. Grav. Theor. Phys. 1, 4 (2025), arXiv:2507.09246 [gr-qc]. [128] Z. Malik, Int. J. Theor. Phys. 64, 314 (2025), arXiv:2508.19178 [gr-qc]. [129] S. V. Bolokhov, arXiv e-prints (2026), arXiv:2603.22310 [gr-qc]. [130] B. C. Lütfüoğlu, Fortsch. Phys. 74, e70074 (2026), arXiv:2510.10579 [gr-qc]. [131] Z. Malik, arXiv e-prints (2024), arXiv:2412."},{"citing_arxiv_id":"2605.12113","ref_index":105,"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":"Lett. B 872, 140082 (2026), arXiv:2510.25969 [gr-qc]. [102] S. V. Bolokhov and M. Skvortsova, JCAP 04, 025 (2025), arXiv:2412.11166 [gr-qc]. [103] Z. Malik, JCAP 04, 042 (2025), arXiv:2412.19443 [gr- qc]. [104] B. C. Lütfüoğlu, A. Shermatov, J. Rayimbaev, M. Maty- oqubov, and O. Sirajiddin, Eur. Phys. J. C 85, 1484 (2025), arXiv:2511.22366 [gr-qc]. [105] R. A. Konoplya and A. Zhidenko, Phys. Rev. D 82, 084003 (2010), arXiv:1004.3772 [hep-th]. [106] R. A. Konoplya, Phys. Lett. B 838, 137674 (2023), arXiv:2210.08373 [gr-qc]."},{"citing_arxiv_id":"2605.11364","ref_index":85,"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":"Zhidenko, Phys. Rev. D 77, 084019 (2008), arXiv:0802.0655 [hep-th]. [82] P. Wongjun, C.-H. Chen, and R. Nakarachinda, Phys. Rev. D 101, 124033 (2020), arXiv:1910.05908 [gr-qc]. [83] R. A. Konoplya and A. Zhidenko, Phys. Rev. D 82, 084003 (2010), arXiv:1004.3772 [hep-th]. [84] M. Skvortsova, Eur. Phys. J. C 85, 854 (2025), arXiv:2411.06007 [gr-qc]. [85] S. Fernando, Gen. Rel. Grav. 48, 24 (2016), arXiv:1601.06407 [gr-qc]. [86] A. Pathrikar, Int. J. Grav. Theor. Phys. 1, 1 (2026), arXiv:2510.01376 [gr-qc]. [87] R. A. Konoplya, Phys. Lett. B 784, 43 (2018), arXiv:1805.04718 [gr-qc]. [88] M. Momennia, S. Hossein Hendi, and F. Soltani Bidgoli, Phys. Lett. B 813, 136028 (2021), arXiv:1807.01792 [hep-th]."},{"citing_arxiv_id":"2605.11013","ref_index":117,"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":"30, 279 (2024), arXiv:2405.15807 [gr-qc]. [113] Z. Malik, Annals Phys. 479, 170046 (2025), arXiv:2409.01561 [gr-qc]. [114] J. P. Arbelaez, arXiv e-prints (2026), arXiv:2601.22340 [gr-qc]. [115] S. V. Bolokhov, Phys. Lett. B 856, 138879 (2024), arXiv:2310.12326 [gr-qc]. [116] A. Dubinsky, Int. J. Grav. Theor. Phys. 1, 2 (2025), arXiv:2507.00256 [gr-qc]. [117] H. Han and B. Gwak, arXiv e-prints (2026), arXiv:2601.18613 [gr-qc]. [118] R. A. Konoplya and A. 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. Malik, JCAP 04, 042 (2025), arXiv:2412.19443 [gr- qc]. [121] B. C. Lütfüoğlu, A. Shermatov, J."},{"citing_arxiv_id":"2605.03659","ref_index":115,"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":"support","context_text":"06007 [gr-qc]. [111] R. A. Konoplya and A. Zhidenko, JCAP 09, 068 (2024), arXiv:2406.11694 [gr-qc]. [112] R. A. Konoplya and A. Zhidenko, Phys. Lett. B 861, 139288 (2025), arXiv:2408.11162 [gr-qc]. [113] R. A. Konoplya and A. Zhidenko, Phys. Rev. D 82, 084003 (2010), arXiv:1004.3772 [hep-th]. [114] Z. Malik, arXiv e-prints (2024), arXiv:2412.13385 [gr- qc]. [115] A. Dubinsky, Mod. Phys. Lett. A 40, 2550111 (2025), arXiv:2412.00625 [gr-qc]. [116] B. C. Lütfüoğlu, Fortsch. Phys. 74, e70074 (2026), arXiv:2510.10579 [gr-qc]. [117] B. C. Lütfüoğlu, Phys. Lett. B 872, 140082 (2026), arXiv:2510.25969 [gr-qc]. [118] B. C. Lütfüoğlu, A. Shermatov, J. Rayimbaev, M. Maty- oqubov, and O. Sirajiddin, Eur. Phys. J. C 85, 1484"},{"citing_arxiv_id":"2605.03137","ref_index":60,"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":"method","top_context_polarity":"use_method","context_text":"4 Im(ω0)2 + Re(ω0)2 (Re(ω0) − Re(ω1))2 16 Im(ω0)4 − 3 Im(ω0) − Im(ω1) 12 Im(ω0) ) + O ( ℓ−3) . (21) This improved relation provides a more accurate esti- mate of the WKB scattering quantity entering Eq. (18) and has already been tested in a number of black-hole and regular-geometry settings, generally showing good agreement even for moderately low multipole numbers [60, 66, 68, 89-99]. At the same time, the correspon- dence inherits the limitations of the WKB picture itself: if the effective potential ceases to be a single barrier, for example by developing a double-well structure [100], or if higher-curvature effects strongly deform the centrifu- gal sector and induce catastrophic instabilities [101-105], the reconstruction of grey-body factors from quasinormal"},{"citing_arxiv_id":"2604.26166","ref_index":52,"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 and gray-body factors of black holes and wormholes in dark matter inspired Weyl gravity, Eur. Phys. J. C85(2025) 486 [2503.16087]. [51] S.V. Bolokhov and M. Skvortsova, Gravitational Quasinormal Modes and Grey-Body Factors of Bonanno-Reuter Regular Black Holes, Int. J. Grav. Theor. Phys.1(2025) 3 [2507.07196]. [52] R.A. Konoplya and A. Zhidenko, Long life of Gauss-Bonnet corrected black holes, Phys. Rev. D82(2010) 084003 [1004.3772]. [53] B.C. 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,"},{"citing_arxiv_id":"2604.25471","ref_index":130,"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":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Murodov, J. Kur- banov, and M. Matyoqubov, (2026), arXiv:2604.14999 [gr-qc]. [126] A. Dubinsky, Mod. Phys. Lett. A 40, 2550111 (2025), arXiv:2412.00625 [gr-qc]. [127] Z. Malik, (2025), arXiv:2510.06689 [gr-qc]. [128] Z. Malik, (2024), arXiv:2412.13385 [gr-qc]. [129] R. A. Konoplya and O. S. Stashko, Phys. Rev. D 111, 084031 (2025), arXiv:2502.05689 [gr-qc]. [130] R. A. Konoplya and A. Zhidenko, Phys. Rev. D 95, 104005 (2017), arXiv:1701.01652 [hep-th]. [131] R. A. Konoplya and A. Zhidenko, JCAP 05, 050 (2017), arXiv:1705.01656 [hep-th]. [132] T. Takahashi and J. Soda, Prog. Theor. Phys. 124, 711 (2010), arXiv:1008.1618 [gr-qc]. [133] G. Dotti and R. J. Gleiser, Class. Quant. Grav. 22, L1 (2005), arXiv:gr-qc/0409005."},{"citing_arxiv_id":"2604.24349","ref_index":79,"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":"D 99, 104060 (2019), arXiv:1904.05341 [gr-qc]. [76] P. Wongjun, C.-H. Chen, and R. Nakarachinda, Phys. Rev. D 101, 124033 (2020), arXiv:1910.05908 [gr-qc]. [77] Z. Malik, Int. J. Grav. Theor. Phys. 2, 3 (2026), arXiv:2603.18887 [gr-qc]. [78] N. Breton, T. Clark, and S. Fernando, Int. J. Mod. Phys. D 26, 1750112 (2017), arXiv:1703.10070 [gr-qc]. 10 [79] R. Karmakar and U. D. Goswami, Phys. Scripta 99, 055003 (2024), arXiv:2310.18594 [gr-qc]. [80] R. A. Konoplya, Gen. Rel. Grav. 34, 329 (2002), arXiv:gr-qc/0109096. [81] R. A. Konoplya and E. Abdalla, Phys. Rev. D 71, 084015 (2005), arXiv:hep-th/0503029. [82] S. V. Bolokhov and M. Skvortsova, Eur. Phys. J. C 86, 374 (2026), arXiv:2508.19989 [gr-qc]."}],"limit":50,"offset":0}