Abstract
In this paper we study the bulk viscous cosmology by considering modified Chaplygin gas in the framework of $$(2+1)$$ -dimensional spacetime. For this we consider various form of bulk viscosity coefficient $$\zeta $$ and then obtain the physical parameters energy density $$\rho $$ , Hubble and deceleration parameters, H and q, respectively. Finally we discuss the stability of the model by using the speed of sound.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
