Electromagnetic parametric instabilities in an ultra-relativistic plasma
- 1 August 1977
- journal article
- research article
- Published by AIP Publishing in Physics of Fluids
- Vol. 20 (8) , 1302-1310
- https://doi.org/10.1063/1.862012
Abstract
The parametric decay of an intense, coherent electromagnetic wave into subluminous electrostatic waves and scattered electromagnetic waves in a homogeneous plasma is studied, with particular attention to the effects of relativistic electron temperature. A mode coupling formalism is developed, from which growth rates for stimulated Raman and Brillouin backscattering in one dimension, and for modulational Raman forward scattering, are derived.Keywords
This publication has 21 references indexed in Scilit:
- Parametric Instabilities in Strongly Relativistic, Plane-Polarized Electromagnetic WavesPhysical Review Letters, 1976
- A multiple pulsar model for quasi-stellar objects and active galactic nucleiThe Astrophysical Journal, 1975
- Self-Modulation and Self-Focusing of Electromagnetic Waves in PlasmasPhysical Review Letters, 1974
- Parametric instability of a relativistically strong electromagnetic wavePhysics of Fluids, 1973
- Instability of a Relativistically Strong Electromagnetic Wave of Circular PolarizationPhysical Review Letters, 1972
- A Search for Discrete Sources of Cosmic Gamma Rays of Energy 10^{11}-10^{12} eVThe Astrophysical Journal, 1972
- New Interpretation of Extragalactic Radio SourcesNature, 1971
- On the Nature of Pulsars. I. TheoryThe Astrophysical Journal, 1969
- Activity in the Crab NebulaThe Astrophysical Journal, 1969
- Parametric Effects of Radiation on a PlasmaPhysical Review B, 1967