KONOPLYA, Roman and A. ZHIDENKO. Analytic expressions for quasinormal modes and grey-body factors in the eikonal limit and beyond. Classical and Quantum Gravity. GB - Spojené království Velké Británie a, 2023, vol. 40, No 24, p. "245005-1"-"245005-16", 16 pp. ISSN 0264-9381. Available from: https://dx.doi.org/10.1088/1361-6382/ad0a52.
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Basic information
Original name Analytic expressions for quasinormal modes and grey-body factors in the eikonal limit and beyond
Authors KONOPLYA, Roman (804 Ukraine, belonging to the institution) and A. ZHIDENKO.
Edition Classical and Quantum Gravity, GB - Spojené království Velké Británie a, 2023, 0264-9381.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher United Kingdom of Great Britain and Northern Ireland
Confidentiality degree is not subject to a state or trade secret
WWW URL
RIV identification code RIV/47813059:19630/23:A0000289
Organization unit Institute of physics in Opava
Doi http://dx.doi.org/10.1088/1361-6382/ad0a52
UT WoS 001121137400001
Keywords in English quasinormal modes;transmission coefficients;grey-body factor;WKB formula;eikonal approximation
Tags RIV24, UF
Tags International impact, Reviewed
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 17/1/2024 14:19.
Abstract
Although the WKB series converges only asymptotically and guarantees the exact result solely in the eikonal regime, we have managed to derive concise analytical expressions for the quasinormal modes and grey-body factors of black holes, expanding beyond the eikonal approximation. Remarkably, these expressions demonstrate unexpectedly strong accuracy. We suggest a comprehensive approach for deriving analytical expressions for grey-body factors and quasinormal modes at various orders beyond the eikonal approximation. Two cases are examined as examples: the Schwarzschild-de Sitter black hole and hairy black holes within the framework of Effective Field Theory. We have publicly shared a generic code that calculates analytical expressions for grey-body factors and quasinormal modes of spherical black holes.
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