Weibel instability with semirelativistic Maxwellian distribution function
Creators
- 1. Salam Chair in Physics, G. C. University Lahore, Lahore, Punjab 54000 (Pakistan)
- 2. Salam Chair in Physics, G. C. University Lahore, Lahore, Punjab 54000 (Pakistan) and Department of Physics, G. C. University Lahore, Lahore, Punjab 54000 (Pakistan)
Description
A macroscopic description of the linear Weibel instability, based on semirelativistic distribution in an unmagnetized plasma is presented. In particular, analytical expressions are derived for the real and imaginary parts of the dielectric constant for the Maxwellian and semirelativistic Maxwellian distribution functions under the conditions of ξ=(ω/kparallelθparallel)>>1 and <<1. The real frequency and the growth rate of the instability for the semirelativistic case now depends upon the factor χ generated from the relativistic term in the distribution function. The presence of χ which is always greater than unity favors the Weibel instability to occur even for the small anisotropy of temperature. As we increase the value of χ large enough that it dominates over other terms, the damping changes into growth. In the limiting case, i.e., χ=1, the results approach the Maxwellian situation
Additional details
Identifiers
- DOI
- 10.1063/1.2749254;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 14
- Journal Issue
- 7
- Journal Page Range
- p. 072106-072106.3
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 39006442
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- ANISOTROPY; BOLTZMANN-VLASOV EQUATION; DAMPING; DISTRIBUTION FUNCTIONS; MAXWELL EQUATIONS; PERMITTIVITY; PLASMA INSTABILITY; RELATIVISTIC PLASMA; RELATIVISTIC RANGE
- Descriptors DEC
- DIELECTRIC PROPERTIES; DIFFERENTIAL EQUATIONS; ELECTRICAL PROPERTIES; ENERGY RANGE; EQUATIONS; FUNCTIONS; INSTABILITY; PARTIAL DIFFERENTIAL EQUATIONS; PHYSICAL PROPERTIES; PLASMA
Optional Information
- Notes
- (c) 2007 American Institute of Physics