KONOPLYA, Roman and A. ZHIDENKO. General black-hole metric mimicking Schwarzschild spacetime. Journal of Cosmology and Astroparticle Physics. GB - Spojené království Velké Británie a, 2023, vol. 2023, No 8, p. "008-1"-"008-18", 18 pp. ISSN 1475-7516. Available from: https://dx.doi.org/10.1088/1475-7516/2023/08/008.
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Basic information
Original name General black-hole metric mimicking Schwarzschild spacetime
Authors KONOPLYA, Roman (804 Ukraine, belonging to the institution) and A. ZHIDENKO.
Edition Journal of Cosmology and Astroparticle Physics, GB - Spojené království Velké Británie a, 2023, 1475-7516.
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:A0000288
Organization unit Institute of physics in Opava
Doi http://dx.doi.org/10.1088/1475-7516/2023/08/008
UT WoS 001089208700008
Keywords in English modified gravity;GR black holes;Gravitational waves in GR and beyond: theory;gravity
Tags RIV24, UF
Tags International impact, Reviewed
Links EF18_054/0014696, research and development project.
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 13/2/2024 14:39.
Abstract
Using the general parametrization of spherically symmetric and asymptotically flat black holes in arbitrary metric theories of gravity and implying that: a) the post-Newtonian constraints are taken into account and b) basic astrophysically relevant characteristics (such as, dominant quasinormal modes, frequency at the innermost stable circular orbit, binding energy, radius of the shadow etc.) are indistinguishable from their Schwarzschild values, we propose a simple metric which depends on three independent parameters (coefficients of the parametrization). Variation of these three parameters can, nevertheless, lead to the two distinctive features. The first is the black-hole temperature, and consequently the Hawking radiation, which can differ a lot from its Schwarzschild limit. The second is the outburst of overtones which become extremely sensitive to small changes of the parameters.
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