Some Bianchi Type Viscous Holographic Dark Energy Cosmological Models in the Brans–Dicke Theory

<div> Pressure of VHDE (<i>P</i><sub><i>vhde</i></sub>) versus redshift (<i>z</i>) for BT-II.</div>

Advances in Astronomy

Figure 1: Some Bianchi Type Viscous Holographic Dark Energy Cosmological Models in the Brans–Dicke Theory 