Locally rotationally symmetric Bianchi type-I cosmological model with dynamical $Lambda$ and $G$ in $f (R)$ gravity
RAKESH RAUSHAN A K SHUKLA R CHAUBEY T SINGH
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In this paper, we have studied the locally rotationally symmetric (LRS) Bianchi type-I cosmological model filled with a bulk viscous cosmological fluid in $f(R)$ gravity in the presence of time-varying gravitational and cosmological constant. We have used the power-law and intermediate scenario for scale factor to obtain thesolution of the field equations. The evolution of temperature of a viscous Universe is also analysed.
RAKESH RAUSHAN1 A K SHUKLA1 R CHAUBEY1 T SINGH2
Volume 97, 2023
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