General-relativistic hydrodynamics of a collisionless plasma in a strong magnetic field

E. G. Tsikarishvili, J. G. Lominadze, A. D. Rogava, and J. I. Javakhishvili
Phys. Rev. A 46, 1078 – Published 1 July 1992
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Abstract

The closed set of general-relativistic hydrodynamical equations describing a strongly magnetized collisionless plasma with an anisotropic pressure tensor is derived. Consideration is based on the ‘‘3+1’’ formulation of magnetohydrodynamics and the orthonormal tetrad technique. The model is the further generalization of the theory of Chew, Goldberger, and Low [Proc. R. Soc. London Ser. A 236, 1204 (1954)] for the general-relativistic case. In ultrarelativistic limit the equations of state are obtained, which differ noticeably from those known previously.

  • Received 29 July 1991

DOI:https://doi.org/10.1103/PhysRevA.46.1078

©1992 American Physical Society

Authors & Affiliations

E. G. Tsikarishvili, J. G. Lominadze, and A. D. Rogava

  • Department of Theoretical Astrophysics, Abastumani Astrophysical Observatory, Tbilisi 380060, Republic of Georgia

J. I. Javakhishvili

  • Department of Physics, Tbilisi State University, Tbilisi 38002, Republic of Georgia

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Vol. 46, Iss. 2 — July 1992

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