Noether symmetry of F(T) cosmology with quintessence and phantom scalar fields

Abstract

In this paper, we investigate the Noether symmetries of $F(T)$ cosmology involving matter and dark energy. In this model, the dark energy is represented by a canonical scalar field with a potential. Two special cases for dark energy are considered including phantom energy and quintessence. We obtain $F(T)\sim T^{3/4},$ and the scalar potential $V(\varphi )\sim {\varphi }^2$ for both models of dark energy and discuss quantum picture of this model. Some astrophysical implications are also discussed.

arXiv comment15 pages,4 figures

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