Abstract
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.
| Original language | English |
|---|---|
| Article number | 027401 |
| Pages (from-to) | 274011-274014 |
| Number of pages | 4 |
| Journal | Physical Review E |
| Volume | 64 |
| Issue number | 2 |
| DOIs | |
| State | Published - 1 Jan 2001 |
ASJC Scopus subject areas
- Statistical and Nonlinear Physics
- Statistics and Probability
- Condensed Matter Physics