We have investigated Bianchi Type V stiff fluid cosmological model with variable gravitational and cosmological constant. To get the exact solution it is assumed that equation of state is P = p – 3 H, =p, where = 0 h, p is the isotropic pressure, is the coefficient of shear viscosity, H the Hubble constant, 0 and h are taken as constants. A, B and C are assumed as the functions of cosmic time t using power law relation. Some other physical and geometrical aspects of the model are also discussed in terms of cosmic time t.
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S. Tinker, "Stiff Fluid Distribution with Variable G and Assuming Power Law Relation in Bianchi type V Viscous Cosmological Model", Journal of Ultra Scientist of Physical Sciences, Volume 29, Issue 10, Page Number 268-275, 2017Copy the following to cite this URL:
S. Tinker, "Stiff Fluid Distribution with Variable G and Assuming Power Law Relation in Bianchi type V Viscous Cosmological Model", Journal of Ultra Scientist of Physical Sciences, Volume 29, Issue 10, Page Number 268-275, 2017Available from: http://www.ultraphysicalsciences.org/paper/857/