Magnetohydrodynamic cosmologies with a Bertotti-Robinson-like limit

Details Magnetohydrodynamic cosmologies with a Bertotti-Robinson-like limit Magnetohydrodynamic cosmologies with a Bertotti-Robinson-like limit

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...316..483p&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 316, May 15, 1987, p. 483-488.

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3

Computational Astrophysics, Cosmology, Magnetohydrodynamics, Maxwell Equation, Conducting Fluids, Electrical Resistivity, Gravitational Collapse, Mathematical Models

Scientific paper

The authors present a class of cosmological solutions of Einstein-Maxwell equations, which have a static Bertotti-Robinson-like model as an asymptotic configuration. The novel feature of the models is the presence of a conductivity current in Maxwell equations characterizing a regime of magnetohydrodynamics. Exact analytical solutions are exhibited, and the solutions may be used as the interior model for the collapse of a self-gravitating bounded fluid with electric conductivity.

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