  We consider the spatially flat Friedmann-Lemaitre-Robertson-Walker space time
in the teleparallel model of gravity and assume that the universe is filled
nearly by cold dark matter and a nonminimally coupled scalar field with a
power-law potential as dark energy. We investigate the possibility that the
universe undergoes a transition from quintessence to phantom phase. An
analytical solution for the scalar field is obtained and necessary conditions
required for such a transition are discussed.
