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.
引用
收藏
相关论文
共 145 条
  • [1] Bennett C.L.(2003)undefined Astrophys. J. Suppl. Ser. 148 1-undefined
  • [2] Spergel D.N.(2003)undefined Astrophys. J. Suppl. Ser. 148 175-undefined
  • [3] Spergel D.N.(2007)undefined Astrophys. J. Suppl. Ser. 170 377-undefined
  • [4] Perlmutter S.(1997)undefined Astrophys. J. 483 565-undefined
  • [5] Perlmutter S.(1998)undefined Nature 391 51-undefined
  • [6] Perlmutter S.(1999)undefined Astrophys. J. 517 565-undefined
  • [7] Riess A.G.(2004)undefined Astrophys. J. 607 665-undefined
  • [8] Riess A.G.(2007)undefined Astrophys. J. 659 98-undefined
  • [9] Eisentein D.J.(2005)undefined Astrophys. J. 633 560-undefined
  • [10] Jain B.(2003)undefined Phys. Rev. Lett. 91 78-undefined
12345678910