eng Ansari Education and Research Society Journal of Ultra Scientist of Physical Sciences October, 2017 29 10 268 275 http://dx.doi.org/10.22147/jusps-B/291003 857 article SEEMA TINKER (seematinker@gmail.com) 1 Department of Mathematics, JECRC University, Jaipur, Rajasthan-303905, India <p style="text-align: justify;">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 &ndash; 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.</p> https://ultraphysicalsciences.org/paper/857/ Bianchi type V universe viscosity, stiff fluid Hubble parameter variation variable G and uf04c