Author:
Sharma Sanjay,Poonia Laxmi,Kumawat Sunil
Abstract
Abstract
We have investigated Bianchi Type VI inflationary model in presence of flat potential to study the accelerating behavior of the physical universe in detail. To obtain the deterministic solution we consider the supplementary relation the component
σ
3
3
of shear tensor
σ
j
i
is proportional to expansion parameter θ which yield to appropriate condition c = (ab)
N
between metric coefficients, where N is non-negative constant. Special case in Bianchi Type VI model provide Bianchi I, III and V space-time. Geometrical and dynamical aspects of models are also discussed in different cases
Subject
General Physics and Astronomy
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