NDLI: Waves in strongly magnetized relativistic plasmas: generally covariant approach.

Content Provider	Semantic Scholar
Author	Gedalin, Michael Melrose, Donald B.
Copyright Year	2001
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.
Starting Page	027401
Ending Page	027401
Page Count	1
File Format	PDF HTM / HTML
DOI	10.1103/PhysRevE.64.027401
Alternate Webpage(s)	http://www.physics.usyd.edu.au/theory/melrose_publications/PDF00s/2001/GMpre01.pdf
Alternate Webpage(s)	http://physics.bgu.ac.il/~gedalin/online/gcm.pdf
Alternate Webpage(s)	http://physics.bgu.ac.il/~gedalin/gedalin_PRE_64_027401_2001.pdf
PubMed reference number	11497751
Alternate Webpage(s)	https://doi.org/10.1103/PhysRevE.64.027401
Journal	Medline
Volume Number	64
Issue Number	2
Part	2
Journal	Physical review. E, Statistical, nonlinear, and soft matter physics
Language	English
Access Restriction	Open
Content Type	Text
Resource Type	Article

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Waves in strongly magnetized relativistic plasmas: generally covariant approach.