  Some anisotropic Bianchi V dark energy models are investigated in a scale
invariant theory of gravity. We consider two non interacting fluids such as
dark energy and a bulk viscous fluid. Dark energy pressure is considered to be
anisotropic in different spatial directions. A dynamically evolving pressure
anisotropy is obtained from the models. The models favour phantom behaviour. It
is observed that, in presence of dark energy, bulk viscosity has no appreciable
affect on the cosmic dynamics.
