KOLOŠ, Martin, Zdeněk STUCHLÍK, Bobomurat AHMEDOV and Arman TURSUNOV. Dynamics of an electric current-carrying string loop near a Schwarzschild black hole embedded in an external magnetic field. Physical Review D. US - Spojené státy americké, 2013, vol. 87, No 12, 7 pp. ISSN 1550-7998. Available from: https://dx.doi.org/10.1103/PhysRevD.87.125003.
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Basic information
Original name Dynamics of an electric current-carrying string loop near a Schwarzschild black hole embedded in an external magnetic field
Authors KOLOŠ, Martin, Zdeněk STUCHLÍK, Bobomurat AHMEDOV and Arman TURSUNOV.
Edition Physical Review D, US - Spojené státy americké, 2013, 1550-7998.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Confidentiality degree is not subject to a state or trade secret
WWW www
Organization unit Faculty of Philosophy and Science in Opava
Doi http://dx.doi.org/10.1103/PhysRevD.87.125003
UT WoS 000319912200010
Keywords in English Cosmic strings; Electromagnetic-fields; Flux tubes
Tags UF
Tags International impact, Reviewed
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 26/1/2021 10:05.
Abstract
We study motion of an electric current-carrying string loop oscillating in the vicinity of the Schwarzschild black hole immersed in an external uniform magnetic field. The dependence of boundaries and different types of motion of the string loop on magnetic field strength is found. The dynamics of the string loop in the Cartesian xy plane depends both on value and direction of the magnetic field and current. It is shown that the magnetic field influence on the behavior of the string loop is quite significant even for weak magnetic field strength. The oscillation of the string loop becomes stronger or weaker in dependence on the direction of the Lorenz force. We illustrate the various regimes of the trajectories of the string loop that can fall down into the black hole, escape to infinity, or be trapped in the finite region near the horizon for the different representative values of the magnetic field. We have also considered the flat spacetime limit as the condition of the escape of th
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