Correspondence between grey-body factors and quasinormal
frequencies for rotating black holes

J 2025

Correspondence between grey-body factors and quasinormal frequencies for rotating black holes

KONOPLYA, Roman a Olexandr ZHYDENKO

Základní údaje

Originální název

Correspondence between grey-body factors and quasinormal frequencies for rotating black holes

Autoři

KONOPLYA, Roman a Olexandr ZHYDENKO

Vydání

Physics Letters B, Netherlands, 2025, 0370-2693

Další údaje

Jazyk

angličtina

Typ výsledku

Článek v odborném periodiku

Obor

10308 Astronomy

Stát vydavatele

Nizozemské království

Utajení

není předmětem státního či obchodního tajemství

Odkazy

URL

Impakt faktor

Impact factor: 4.500 v roce 2024

Označené pro přenos do RIV

Ano

Organizační jednotka

Fyzikální ústav v Opavě

DOI

https://doi.org/10.1016/j.physletb.2025.139288

UT WoS

001421461700001

EID Scopus

2-s2.0-85216233343

Klíčová slova anglicky

oscillation frequencies ; quasinormal modes; grey-body factors; black holes

Štítky

RIV26, UF

Příznaky

Mezinárodní význam, Recenzováno

Změněno: 25. 2. 2026 13:17, Mgr. Pavlína Jalůvková

Anotace

V originále

Although the proper oscillation frequencies of black holes (quasinormal modes) and the grey-body factors, which determine the scattering properties of black holes, represent two distinct spectral problems with different boundary conditions, a recent study has revealed an intrinsic connection between these quantities. We have shown that the correspondence between grey-body factors and quasinormal modes, previously established for spherically symmetric and asymptotically flat black holes, also extends to general parametrized axially symmetric black holes. This correspondence is limited to non-superradiant waves.

Citovat

KONOPLYA, Roman a Olexandr ZHYDENKO. Correspondence between grey-body factors and quasinormal frequencies for rotating black holes. Physics Letters B. Netherlands, 2025, roč. 861, February 2025, s. "139288-1"-"139288-6", 6 s. ISSN 0370-2693. Dostupné z: https://doi.org/10.1016/j.physletb.2025.139288.

@article{90249,
   author = {Konoplya, Roman and Zhydenko, Olexandr},
   article_location = {Netherlands},
   article_number = {February 2025},
   doi = {https://doi.org/10.1016/j.physletb.2025.139288},
   keywords = {oscillation frequencies ; quasinormal modes; grey-body factors; black holes},
   language = {eng},
   issn = {0370-2693},
   journal = {Physics Letters B},
   title = {Correspondence between grey-body factors and quasinormal frequencies for rotating black holes},
   url = {https://www.sciencedirect.com/science/article/pii/S0370269325000486?pes=vor&utm_source=clarivate&getft_integrator=clarivate},
   volume = {861},
   year = {2025}
}

TY  - JOUR
ID  - 90249
AU  - Konoplya, Roman - Zhydenko, Olexandr
PY  - 2025
TI  - Correspondence between grey-body factors and quasinormal frequencies for rotating black holes
JF  - Physics Letters B
VL  - 861
IS  - February 2025
SP  - "139288-1"-"139288-6"
EP  - "139288-1"-"139288-6"
SN  - 03702693
KW  - oscillation frequencies
KW  - quasinormal modes
KW  - grey-body factors
KW  - black holes
UR  - https://www.sciencedirect.com/science/article/pii/S0370269325000486?pes=vor&utm_source=clarivate&getft_integrator=clarivate
N2  - Although the proper oscillation frequencies of black holes (quasinormal modes) and the grey-body factors, which determine the scattering properties of black holes, represent two distinct spectral problems with different boundary conditions, a recent study has revealed an intrinsic connection between these quantities. We have shown that the correspondence between grey-body factors and quasinormal modes, previously established for spherically symmetric and asymptotically flat black holes, also extends to general parametrized axially symmetric black holes. This correspondence is limited to non-superradiant waves.
ER  -

KONOPLYA, Roman a Olexandr ZHYDENKO. Correspondence between grey-body factors and quasinormal frequencies for rotating black holes. \textit{Physics Letters B}. Netherlands, 2025, roč.~861, February 2025, s.~''139288-1''-''139288-6'', 6 s. ISSN~0370-2693. Dostupné z: https://doi.org/10.1016/j.physletb.2025.139288.

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