Kinetic theory of the generation of magnetic fields in the radiation-dominated stage of expansion of the universe

Details Kinetic theory of the generation of magnetic fields in the radiation-dominated stage of expansion of the universe Kinetic theory of the generation of magnetic fields in the radiation-dominated stage of expansion of the universe

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992svphj..35...98z&link_type=abstract

Soviet Physics Journal, Volume 35, Issue 1, pp.98-102

Physics

Scientific paper

The system of linearized Einstein and Maxwell equations and a kinetic equation with model collision integral for the cosmological plasma are used to calculate the magnetic field generated by solenoidal perturbations in the radiation-dominated stage of expansion of the universe. The magnetic field is generated by two effects — the Harrison effect and a new effect due to kinetic processes. The second effect contributes to the magnetic field if solenoidal gravitational perturbations exist from the very beginning of the radiation-dominated stage.

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