Microscopic model for relativistic hydrodynamics of ideal plasmas
Pavel A. Andreev

TL;DR
This paper derives a relativistic hydrodynamic model for ideal plasmas from microscopic principles, introducing new variables without nonrelativistic analogs, and presents the final equations in a mean-field approximation.
Contribution
It develops a microscopic derivation of relativistic hydrodynamics for ideal plasmas, revealing new variables unique to the relativistic regime.
Findings
New relativistic-hydrodynamic variables identified
Derived equations reduce to classical variables in nonrelativistic limit
Final model presented in the monopole mean-field approximation
Abstract
Relativistic hydrodynamics of classic plasmas is derived from the microscopic model in the limit of ideal plasmas. The chain of equations is constructed step by step starting from the concentration evolution. It happens that the energy density and the momentum density do not appear at such approach, but new relativistic-hydrodynamic variables appear in the model. These variables has no nonrelativistic analogs, but they are reduced to the concentration, the particle current, the pressure (the flux of the particle current) if relativistic effects are dropped. These variables are reduced to functions of the concentration, the particle current, the pressure if the thermal velocities are dropped in compare with the relativistic velocity field. Final equations are presented in the monopole limit of the meanfield (the selfconsistent field) approximation. Hence, the contributions of the…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Dust and Plasma Wave Phenomena
