The general class of Bianchi cosmological models with dark energy and variable $\Lambda$ and $G$ in viscous cosmology
R CHAUBEY A K SHUKLA RAKESH RAUSHAN
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The general class of Bianchi cosmological models with dark energy in the form of modified Chaplygin gas with variable $\Lambda$ and $G$ and bulk viscosity have been considered. We discuss three types of average scalefactor by using a special law for deceleration parameter which is linear in time with negative slope. The exact solutions to the corresponding field equations are obtained. We obtain the solution of bulk viscosity ($\xi$ ), cosmologicalconstant ($\Lambda$), gravitational parameter ($G$) and deceleration parameter ($q$) for different equations of state. The model describes an accelerating Universe for large value of time $t$ , wherein the effective negative pressure induced by Chaplygin gas and bulk viscous pressure are driving the acceleration.
R CHAUBEY1 A K SHUKLA1 RAKESH RAUSHAN1
Volume 97, 2023
Continuous Article Publishing mode
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