TROVA, Audrey, Kris SCHROVEN, Eva HACKMANN, Vladimír KARAS, Jiří KOVÁŘ and Petr SLANÝ. Equilibrium configurations of a charged fluid around a Kerr black hole. Physical Review D. 2018, vol. 97, No 10, p. "104019-1"-"104019-13", 13 pp. ISSN 2470-0010. Available from: https://dx.doi.org/10.1103/PhysRevD.97.104019.
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Basic information
Original name Equilibrium configurations of a charged fluid around a Kerr black hole
Authors TROVA, Audrey (250 France), Kris SCHROVEN (276 Germany), Eva HACKMANN (276 Germany), Vladimír KARAS (203 Czech Republic), Jiří KOVÁŘ (203 Czech Republic, guarantor, belonging to the institution) and Petr SLANÝ (203 Czech Republic, belonging to the institution).
Edition Physical Review D, 2018, 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/47813059:19240/18:A0000264
Organization unit Faculty of Philosophy and Science in Opava
Doi http://dx.doi.org/10.1103/PhysRevD.97.104019
UT WoS 000433027300003
Keywords in English Kerr black hole; electrically charged perfect fluid; equilibrium configuration
Tags International impact, Reviewed
Links GB14-37086G, research and development project.
Changed by Changed by: RNDr. Jan Hladík, Ph.D., učo 25379. Changed: 4/4/2019 12:55.
Abstract
Equilibrium configurations of electrically charged perfect fluid surrounding a central rotating black hole endowed with a test electric charge and embedded in a large-scale asymptotically uniform magnetic field are presented. Following our previous studies considering the central black hole to be nonrotating, we show that in the rotating case conditions for the configurations existence change according to the spin of the black hole. We focus our attention on the charged fluid in rigid rotation, which can form toroidal configurations centered in the equatorial plane or the ones hovering above the black hole, along the symmetry axis. We conclude that a nonzero value of spin changes the existence conditions and the morphology of the solutions significantly. In the case of fast rotation, the morphology of the structures is close to an oblate shape.
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