Detailed Information on Publication Record
2018
Electromagnetic perturbations of black holes in general relativity coupled to nonlinear electrodynamics
TOSHMATOV, Bobir, Zdeněk STUCHLÍK, Jan SCHEE and Bobomurat AHMEDOVBasic information
Original name
Electromagnetic perturbations of black holes in general relativity coupled to nonlinear electrodynamics
Authors
TOSHMATOV, Bobir (860 Uzbekistan, guarantor, belonging to the institution), Zdeněk STUCHLÍK (203 Czech Republic, belonging to the institution), Jan SCHEE (203 Czech Republic, belonging to the institution) and Bobomurat AHMEDOV (860 Uzbekistan)
Edition
Physical Review D, 2018, 2470-0010
Other information
Language
English
Type of outcome
Článek v odborném periodiku
Field of Study
10308 Astronomy
Country of publisher
United States of America
Confidentiality degree
není předmětem státního či obchodního tajemství
References:
RIV identification code
RIV/47813059:19240/18:A0000265
Organization unit
Faculty of Philosophy and Science in Opava
UT WoS
000432961800008
Keywords in English
general relativity; black holes; nonlinear electrodynamics; electromagnetic perturbations
Tags
International impact, Reviewed
Links
GB14-37086G, research and development project.
Změněno: 4/4/2019 09:38, RNDr. Jan Hladík, Ph.D.
Abstract
V originále
The electromagnetic (EM) perturbations of the black hole solutions in general relativity coupled to nonlinear electrodynamics (NED) are studied for both electrically and magnetically charged black holes, assuming that the EM perturbations do not alter the spacetime geometry. It is shown that the effective potentials of the electrically and magnetically charged black holes related to test perturbative NED EM fields are related to the effective metric governing the photon motion, contrary to the effective potential of the linear electrodynamic (Maxwell) field that is related to the spacetime metric. Consequently, corresponding quasinormal (QN) frequencies differ as well. As a special case, we study new family of the NED black hole solutions which tend in the weak field limit to the Maxwell field, giving the Reissner-Nordstrom (RN) black hole solution. We compare the NED Maxwellian black hole QN spectra with the RN black hole QN spectra.