Relativistic two fluid plasmas in the vicinity of a Schwarzschild black hole-Local approximation. II

Details Relativistic two fluid plasmas in the vicinity of a Schwarzschild black hole-Local approximation. II Relativistic two fluid plasmas in the vicinity of a Schwarzschild black hole-Local approximation. II

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995phrvd..51.6677b&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 51, Issue 12, 15 June 1995, pp.6677-6691

Astronomy and Astrophysics

Astrophysics

19

Magnetohydrodynamics And Plasmas, Relativity And Gravitation, Black Holes

Scientific paper

The 3+1 split of general relativity is used in a preliminary investigation of waves propagating in a plasma influenced by the gravitational field of a Schwarzschild black hole. The relativistic two fluid equations have been reformulated, as explained in an earlier paper, to take account of gravitational effects due to the event horizon. Here, a local approximation is used to investigate the one-dimensional radial propagation of longitundial waves. A study is also included of the two stream instability in view of its importance in astrophysics. Dispersion relations are obtained for these waves and solved numerically for the wave number k.

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