Аннотации:
We focus on a viable teleparallel cosmological model with a scalar field in a flat
Friedman-Robertson-Walker universe. The Lagrangian and equations of motion are obtained.
The case of an inhomogeneous viscous dark energy is considered and the cosmological
parameters associated with the viscosity parameter are determined. It is shown that when
considering constant viscosity and state parameter, the Universe expands exponentially
