An analytic solution of the Boltzmann equation in the presence of self-generated magnetic fields in astrophysical plasmas |
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| Institution: | 1. Department of Mathematics, Central University of Karnataka, Kalaburagi 585311, India;2. Discipline of Chemical Engineering, University of Newcastle, Callaghan, NSW 2308, Australia;1. Institute of Nuclear Physics Polish Academy of Sciences, ul. Radzikowskiego 152, Cracow 31-342, Poland;2. Institute of Plasma Physics of the Czech Academy of Sciences, Za Slovankou 1782/3, Prague 182 00, Czech Republic;1. Department of Energy Science and Engineering, Indian Institute of Technology Delhi, Hauz Khas, New Delhi 110016, India;2. The University of Queensland Australia, Australia;1. Computational Analysis Division, Bhabha Atomic Research Centre (BARC), Visakhapatnam, India;2. High Pressure & Synchrotron Radiation Physics Division, Bhabha Atomic Research Centre (BARC), Mumbai, India |
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| Abstract: | 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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