Magnetohydrodynamic cosmologies

Details Magnetohydrodynamic cosmologies Magnetohydrodynamic cosmologies

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...380..330p&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 380, Oct. 20, 1991, p. 330-333.

Statistics

Computation

2

Astronomical Models, Computational Astrophysics, Cosmic Plasma, Gravitational Collapse, Plasma-Electromagnetic Interaction, Stellar Interiors, Ideal Fluids, Magnetohydrodynamics, Stellar Magnetic Fields, Thermodynamic Equilibrium

Scientific paper

A class of cosmological models in magnetohydrodynamic regime extending and completing the results of a previous paper is analyzed. The material content of the models is a perfect fluid plus electromagnetic fields. The fluid is neutral on average but admits an electrical current which satisfies Ohm's law. All models fulfill the physical requirements of near-equilibrium thermodynamics and can be favorably used as a more realistic description of the interior of a collapsing star in a magnetohydrodynamic regime with or without a magnetic field.

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