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

被引：0
作者：
Mubasher Jamil
D. Momeni
R. Myrzakulov
机构：
[1] National University of Sciences and Technology (NUST),Center for Advanced Mathematics and Physics (CAMP)
[2] Eurasian National University,Eurasian International Center for Theoretical Physics
来源：
The European Physical Journal C | 2012年 / 72卷
关键词：
Dark Energy; Scalar Field; Quantum Cosmology; Cosmic Acceleration; Hamiltonian Constraint;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
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)∼T3/4, and the scalar potential V(ϕ)∼ϕ2 for both models of dark energy and discuss quantum picture of this model. Some astrophysical implications are also discussed.
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