Waves in strongly magnetized relativistic plasmas: Generally covariant approach

Details Waves in strongly magnetized relativistic plasmas: Generally covariant approach Waves in strongly magnetized relativistic plasmas: Generally covariant approach

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001phrve..64b7401g&link_type=abstract

Physical Review E (Statistical, Nonlinear, and Soft Matter Physics), Volume 64, Issue 2, August 2001, id.027401

Physics

4

Relativistic Plasmas, Magnetized Plasmas, Magnetohydrodynamics And Plasmas, Late Stages Of Stellar Evolution

Scientific paper

A dispersion relation for long waves in strongly magnetized multifluid plasma in a curved spacetime is derived in a covariant form. A generally covariant form for the ray equations is obtained. The results are applicable to ray propagation in relativistic plasmas in the vicinity of strongly gravitating (black holes) or rapidly rotating (pulsars) systems.

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