We consider the spatially flat Friedmann-Lemaitre-Robertson-Walker space-time in the teleparallel model of gravity and assume that the Universe is nearly filled 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.
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H. Mohseni Sadjadi (2013) studied this question.
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