Viscous Dark Energy and Phantom Field in An Anisotropic Universe
  In this paper we have investigated the general form of viscous and
non-viscous dark energy equation of state (EoS) parameter in the scope of
anisotropic Bianchi type I space-time. We show that the presence of bulk
viscosity causes transition of $\omega^{de}$ from quintessence to phantom but
the phantom state is an unstable state (as expected) and EoS of DE tends to
$-1$ at late time. Then we show this phantomic description of the viscous dark
energy and reconstruct the potential of the phantom scalar field. It is found
that bulk viscosity pushes the universe to a darker region. We have also shown
that at late time $q\sim-\Omega^{de}$.
