An analytic solution of the Boltzmann equation in the presence of self-generated magnetic fields in astrophysical plasmas

Details An analytic solution of the Boltzmann equation in the presence of self-generated magnetic fields in astrophysical plasmas An analytic solution of the Boltzmann equation in the presence of self-generated magnetic fields in astrophysical plasmas

1998-07-12

arxiv.org/abs/astro-ph/9807116v1

Phys.Lett. A246 (1998) 436-440

Astronomy and Astrophysics

Astrophysics

4 pages, no figure, in REVTeX, accepted for publication in Phys. lett. A

Scientific paper

10.1016/S0375-9601(98)00539-8

Through relating a self-generated magnetic field to the regular motion of
free electrons that is responsible for the magnetic field generation in
astrophysical plasmas, we solve the Boltzmann kinetic equation in the presence
of the self-generated magnetic fields to obtain a steady-state, collisional
invariant analytic solution of the equation.

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