Abstract:
In this paper, we investigate the Noether symmetries of F (T ) cosmology in-volving 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 phan-tom energy and quintessence. We obtain F (T ) ∼ T
3/4
, and the scalar potential V (φ) ∼ φ
2
for both models of dark energy and discuss quantum picture of this model. Some astrophys-ical implications are also discussed.
