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Role of electric charge in shaping equilibrium configurations of fluid tori encircling black holes

Jiří Kovář*, Petr Slaný, and Zdeněk Stuchlík

Vladimír Karas

Claudio Cremaschini

John C. Miller

  • Institute of Physics, Faculty of Philosophy and Science, Silesian University in Opava Bezručovo nám. 13, CZ-74601 Opava, Czech Republic

  • Astronomical Institute, Academy of Sciences, Boční II, CZ-14131 Prague, Czech Republic

  • SISSA & INFN, Via Bonomea 265, I-34136 Trieste, Italy

  • SISSA & INFN, Via Bonomea 265, I-34136 Trieste, Italy and Department of Physics (Astrophysics), University of Oxford, Keble Road, Oxford OX1 3RH, U.K.

  • *Jiri.Kovar@fpf.slu.cz

Phys. Rev. D 84, 084002 – Published 4 October, 2011

DOI: https://doi.org/10.1103/PhysRevD.84.084002

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 and electromagnetic 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 around Reissner-Nordström black holes and compare them with equivalent configurations of electrically neutral tori.

See Also

Charged perfect fluid tori in strong central gravitational and dipolar magnetic fields

Jiří Kovář, Petr Slaný, Claudio Cremaschini, Zdeněk Stuchlík, Vladimír Karas, and Audrey Trova
Phys. Rev. D 93, 124055 (2016)

Article Text

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