Abstract
The present paper deals with strange quark matter i.e. ( 4 ) in the presence of variable cosmological term in Bianchi VI universe. Here we adopt the physical conditions (i)The shear scalar is proportional to expansion scalar and ( ii ) The time dependent cosmological term of the type 2 for the simplification of field equations. We observed some cosmological parameters such as deceleration parameter, quark density, quark pressure etc. Lastly we conclude with the discussion of cosmological perturbations of resultant universe. Also graphs are plotted for the detail study of the resultant model.
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Schedule a callMore From: SAMRIDDHI : A Journal of Physical Sciences, Engineering and Technology
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