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

<div> The pressure of VHDE(<i>P</i><sub><i>vhde</i></sub>) versus redshift (<i>z</i>) for BT-IX.</div>

Advances in Astronomy

Figure 3: Some Bianchi Type Viscous Holographic Dark Energy Cosmological Models in the Brans–Dicke Theory 