TURIMOV, Bobur, Bobir TOSHMATOV, Bobomurot AHMEDOV and Zdeněk STUCHLÍK. Quasinormal modes of magnetized black hole. Physical Review D. 2019, vol. 100, No 8, p. "084038-1"-"084038-8", 8 pp. ISSN 2470-0010. Available from: https://dx.doi.org/10.1103/PhysRevD.100.084038.
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Basic information
Original name Quasinormal modes of magnetized black hole
Authors TURIMOV, Bobur (860 Uzbekistan, guarantor, belonging to the institution), Bobir TOSHMATOV (203 Czech Republic, belonging to the institution), Bobomurot AHMEDOV (860 Uzbekistan) and Zdeněk STUCHLÍK (203 Czech Republic, belonging to the institution).
Edition Physical Review D, 2019, 2470-0010.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher United States of America
Confidentiality degree is not subject to a state or trade secret
WWW URL
RIV identification code RIV/47813059:19240/19:A0000413
Organization unit Faculty of Philosophy and Science in Opava
Doi http://dx.doi.org/10.1103/PhysRevD.100.084038
UT WoS 000490753000009
Keywords in English magnetized black hole; quasinormal modes; stability
Tags Erasmus, , GA19-03950S, RCTPA, RIVOK, SGS12-2019
Tags International impact, Reviewed
Links GA19-03950S, research and development project.
Changed by Changed by: Ing. Petra Skoumalová, učo 50554. Changed: 21/4/2020 10:27.
Abstract
We investigate a charged, massive scalar field around a static, spherically symmetric black hole immersed into an external asymptotically uniform magnetic field B. It is shown that for given multipole number l there are 2l + 1 numbers of modes due to the Zeeman effect appearing by an interaction of the external magnetic and charged scalar fields introducing an effective mass of the scalar field mu_(eff) = square root (mu^2 - mqB) where m is the azimuthal number and q is the charge coupling constant. We calculate threshold value of effective mass in which quasinormal modes are arbitrarily long lived and beyond that value quasinormal modes vanish. In the case of mqB < 0 quasinormal modes are longer lived with larger oscillation frequencies. Whenever, magnetic and massive scalar fields satisfies condition mu^(2)_(eff) < 0, an instability appears, i.e., if qB > 0 or qB < 0 there is an instability for the values of azimuthal number m > mu^2/qB or m < mu^2/qB, respectively.
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