1. Semicollisional heat flux in relativistic plasmas.
- Author
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Bendib-Kalache, K. and Bendib, A.
- Subjects
- *
KNUDSEN flow , *HEAT flux , *INERTIAL confinement fusion , *RELATIVISTIC plasmas , *PLASMA instabilities , *THERMAL conductivity - Abstract
The generalized heat flux in plasmas is analytically calculated using the linear relativistic Fokker–Planck equation. The thermal conductivity and the convective heat flux coefficients are calculated for arbitrary collisionality and plasma temperature. The role of relativistic effects coupled with nonlocal effects on the transport is studied. It was found that the thermal conductivity coefficient decreases with increasing Knudsen number and increasing relativistic effects. In addition, the convective heat flux coefficient is significant in the collisionless range and for the weakly relativistic regime. In particular, in laser-created plasmas, the damping of the plasma eigenmodes should increase with increasing relativistic effects and decrease with increasing nonlocal effects. Consequently, the growth rates of parametric instabilities in plasmas created in the context of inertial confined fusion are expected to be reduced by relativistic effects. [ABSTRACT FROM AUTHOR]
- Published
- 2025
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