Modeling of Accelerating Universe with Bulk Viscous Fluid in Bianchi V Space?Time

In this paper, we have investigated a bulk viscous anisotropic Universe and constrained its model parameters with recent $H(z)$ Pantheon compilation data. Using cosmic chronometric technique, estimate the present value of Hubble's constant as $H_{0} = 69.39 \pm 1.54~km~s^{-1}Mpc^{-1}$, $70.016 1.65~km~s^{-1}Mpc^{-1}$ $69.36 1.42~km~s^{-1}Mpc^{-1}$ by bounding our derived data, joint data respectively. The age is specified $t_0= 0.9796H_0^{-1}\sim 13.79$ Gyrs. favours transitioning transition red-shift $z_{t} 0.73$. We reconstructed jerk parameter using observational sets. From analysis parameter, it observed that, shows marginal departure from concordance $\Lambda$CDM model.