Cosmological viscous fluid models in the presence of electromagnetic field and zero-mass scalar field

Details Cosmological viscous fluid models in the presence of electromagnetic field and zero-mass scalar field Cosmological viscous fluid models in the presence of electromagnetic field and zero-mass scalar field

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.150..309t&link_type=abstract

Astrophysics and Space Science, Volume 150, Issue 2, pp.309-316

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

The problem of electromagnetic field interacting with viscous fluid without and with zero-mass scalar field has been studied. It has been shown that electromagnetic field cannot interact with viscous fluid for spherically-symmetric Robertson-Walker metric. Exact solutions corresponding to the problem of electromagnetic field interactions in presence of viscous fluid and zero-mass scalar field have been obtained subject to various physical conditions. They present a scope for the study of imperfect fluid FRW models showing the existence of the electromagnetic field due to the presence of zero-mass scalar field.

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