KARAS, Vladimír and Zdeněk STUCHLÍK. Magnetized Black Holes: Interplay between Charge and Rotation. Universe. Switzerland, 2023, vol. 9, No 6, p. "267-1"-"267-10", 10 pp. ISSN 2218-1997. Available from: https://dx.doi.org/10.3390/universe9060267.
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Basic information
Original name Magnetized Black Holes: Interplay between Charge and Rotation
Authors KARAS, Vladimír (203 Czech Republic) and Zdeněk STUCHLÍK (203 Czech Republic, belonging to the institution).
Edition Universe, Switzerland, 2023, 2218-1997.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher Switzerland
Confidentiality degree is not subject to a state or trade secret
WWW URL
RIV identification code RIV/47813059:19630/23:A0000260
Organization unit Institute of physics in Opava
Doi http://dx.doi.org/10.3390/universe9060267
UT WoS 001017934600001
Keywords in English black holes;electromagnetic fields;general relativity;microquasars;supermassive black holes
Tags RIV24, UF
Tags International impact, Reviewed
Links GX21-06825X, research and development project.
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 18/3/2024 13:32.
Abstract
Already in the cornerstone works on astrophysical black holes published as early as in the 1970s, Ruffini and collaborators have revealed the potential importance of an intricate interaction between the effects of strong gravitational and electromagnetic fields. Close to the event horizon of the black hole, magnetic and electric lines of force become distorted and dragged even in a purely electro-vacuum system. Moreover, as the plasma effects inevitably arise in any astrophysically realistic environment, particles of different electric charges can separate from each other, become accelerated away from the black hole or accreted onto it, and contribute to the net electric charge of the black hole. From the point of principle, the case of super-strong magnetic fields is of particular interest, as the electromagnetic field can act as a source of gravity and influence spacetime geometry. In a brief celebratory note, we revisit aspects of rotation and charge within the framework of exact (asymptotically non-flat) solutions of mutually coupled Einstein-Maxwell equations that describe magnetized, rotating black holes.
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