KOVÁŘ, Jiří, Petr SLANÝ and Zdeněk STUCHLÍK. Role of electric charge in shaping equilibrium configurations of fluid tori encircling black holes. Physical Review D. US - Spojené státy americké, 2011, vol. 84, No 8, p. 1-15, 14 pp. ISSN 1550-7998. Available from: https://dx.doi.org/10.1103/PhysRevD.84.084002.
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Basic information
Original name Role of electric charge in shaping equilibrium configurations of fluid tori encircling black holes
Authors KOVÁŘ, Jiří, Petr SLANÝ and Zdeněk STUCHLÍK.
Edition Physical Review D, US - Spojené státy americké, 2011, 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
Organization unit Faculty of Philosophy and Science in Opava
Doi http://dx.doi.org/10.1103/PhysRevD.84.084002
UT WoS 000296524300003
Keywords in English Toroidal magnetic-field, compact object, thick discs, cosmological constant, magnetofluid
Tags UF
Tags International impact, Reviewed
Links LC06014, research and development project. MSM4781305903, plan (intention).
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 13/1/2021 11:04.
Abstract
Astrophysical fluids may acquire nonzero electrical charge because of strong irradiation or charge separation in a magnetic field. In this case, electromagnetic and gravitational forces may act together and produce new equilibrium configurations, which are different from the uncharged ones. Following our previous studies of charged test particles and uncharged perfect fluid tori encircling compact objects, we introduce here a simple test model of a charged perfect fluid torus in strong gravitational andelectromagnetic fields. In contrast to ideal magnetohydrodynamic models, we consider here the opposite limit of negligible conductivity, where the charges are tied completely to the moving matter. This is an extreme limiting case which can provide a useful reference against which to compare subsequent more complicated astrophysically motivated calculations. To clearly demonstrate the features of our model, we construct three-dimensional axisymmetric charged toroidal configurations aroun
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