TOSHMATOV, Bobir and Zdeněk STUCHLÍK. Slowly decaying resonances of massive scalar fields around Schwarzschild-de Sitter black holes. European Physical Journal Plus. 2017, vol. 132, No 7, p. „324-1“-„324-9“, 9 pp. ISSN 2190-5444. Available from: https://dx.doi.org/10.1140/epjp/i2017-11596-3.
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Basic information
Original name Slowly decaying resonances of massive scalar fields around Schwarzschild-de Sitter black holes
Authors TOSHMATOV, Bobir (860 Uzbekistan, guarantor, belonging to the institution) and Zdeněk STUCHLÍK (203 Czech Republic, belonging to the institution).
Edition European Physical Journal Plus, 2017, 2190-5444.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher Germany
Confidentiality degree is not subject to a state or trade secret
WWW European Physical Journal Plus
RIV identification code RIV/47813059:19240/17:A0000012
Organization unit Faculty of Philosophy and Science in Opava
Doi http://dx.doi.org/10.1140/epjp/i2017-11596-3
UT WoS 000406285300001
Keywords in English quasinormal modes; massive scalar fields; black holes; cosmic repulsion
Tags International impact, Reviewed
Links GB14-37086G, research and development project.
Changed by Changed by: RNDr. Jan Hladík, Ph.D., učo 25379. Changed: 9/4/2018 05:29.
Abstract
We study in special limiting cases quasinormal modes of massive scalar fields in the Schwarzschild-de Sitter black hole backgrounds. We determine the lower limit on the mass parameter of the scalar field that allows the waves with quasinormal frequencies to propagate to infinity, showing that it depends on the spacetime parameters only. Then we discuss in the large multipole number limit quasinormal modes, whose frequencies can be directly related to the unstable circular photon geodesics. In the large scalar mass approximation, we demonstrate the new interesting phenomenon of slowly decaying resonances, that are strongly related to the maximum of the effective potential of the massive scalar field, which is located at the static radius of the Schwarzschild-de Sitter spacetimes, where the cosmic repulsion is just balanced by the black hole attraction.
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