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

<div> Deceleration parameter (<i>q</i>) versus redshift (<i>z</i>) for BT-VIII.</div>

Advances in Astronomy

Figure 10: Some Bianchi Type Viscous Holographic Dark Energy Cosmological Models in the Brans–Dicke Theory 