{"total":12,"items":[{"citing_arxiv_id":"2605.21533","ref_index":106,"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":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.12113","ref_index":78,"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":"Arbelaez, arXiv e-prints (2026), arXiv:2601.22340 [gr-qc]. 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Dolan,"},{"citing_arxiv_id":"2601.17906","ref_index":157,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Telling tails and quasi-resonances in the vicinity of Dymnikova regular black hole","primary_cat":"gr-qc","submitted_at":"2026-01-25T16:54:41+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Massive scalar perturbations on the Dymnikova regular black hole exhibit growing oscillation frequencies, reduced damping rates leading to quasi-resonances, power-law oscillatory tails, and mass-dependent suppression of grey-body factors.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2510.27320","ref_index":32,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"The quasinormal modes of the rotating quantum corrected black holes","primary_cat":"gr-qc","submitted_at":"2025-10-31T09:47:10+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"The work calculates scalar quasinormal mode spectra for a rotating quantum-corrected black hole and constructs a methodological pipeline to infer the quantum correction parameter from gravitational-wave ringdown data using informative priors.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}