Inhomogeneous perfect fluid universe with electromagnetic field

Details Inhomogeneous perfect fluid universe with electromagnetic field Inhomogeneous perfect fluid universe with electromagnetic field

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ap%26ss.312..267p&link_type=abstract

Astrophysics and Space Science, Volume 312, Issue 3-4, pp. 267-273

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

Cylindrically symmetric inhomogeneous cosmological model for perfect fluid distribution with electromagnetic field is obtained. The source of the magnetic field is due to an electric current produced along the z-axis. F 12 is the non-vanishing component of electromagnetic field tensor. To get the deterministic solution, it has been assumed that the expansion θ in the model is proportional to the shear σ. Physical and geometric aspects of the models are also discussed in presence and absence of magnetic field.

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