Vol. 4 (04) pp. 131-134 DOI: 10.21474/IJAR01/246

LOCALLY-ROTATIONALLY SYMMETRIC BIANCHI TYPE-V COSMOLOGICAL MODEL IN PRESENCE OF PERFECT FLUID AND MAGNETIC FLUX WITH VARIABLE MAGNETIC PERMEABILITY.

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  • Department of Mathematics, Arts, Science and Commerce College, Chikhaldara, Dist. Amravati (M.S.), India -444807.
  • Department of Mathematics, P. R. Patil College of Engineering and Technology, Amravati (M.S.), India -444602.
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Abstract

In this paper, we have investigated the nature of locally-rotationally symmetric Bianchi type-V cosmological model in presence of perfect fluid and magnetic flux in general relativity. We have considered the magnetic permeability as variable quantity. The magnetic field is due to an electric current produced along x-axis, F_23 is the only non-vanishing component of electromagnetic field tensor F_ij. To get the deterministic solution, it has been assumed that ρ=-p. We also discuss the physical and geometrical properties of model.

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How to Cite This Article

PATIL V. R and BHOJNE S. A. (2016); LOCALLY-ROTATIONALLY SYMMETRIC BIANCHI TYPE-V COSMOLOGICAL MODEL IN PRESENCE OF PERFECT FLUID AND MAGNETIC FLUX WITH VARIABLE MAGNETIC PERMEABILITY., Int. J. of Adv. Res., 4 (04), 131-134, ISSN 2320-5407. DOI: https://doi.org/10.21474/IJAR01/246

Corresponding Author

Ms. SARIKA A. BHOJNE

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