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. - See more at:
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