Scalar field induced dynamical evolution in teleparallel gravity

被引:4
|
作者
Mishra, B. [1 ]
Kadam, S. A. [1 ]
Tripathy, S. K. [2 ]
机构
[1] Birla Inst Technol & Sci Pilani, Dept Math, Hyderabad Campus, Hyderabad 500078, India
[2] Indira Gandhi Inst Technol, Dept Phys, Sarang 759146, Odisha, India
关键词
D O I
10.1016/j.physletb.2024.138968
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper, we investigate the role of scalar field potentials in the dynamical evolution of the Universe. A gravity theory with a non-minimally coupled scalar field with torsion in the geometrical action simulating effective dark energy is considered to study an extended matter bounce scenario. The dynamical behaviour of the equation of state parameter has been studied near the bouncing epoch. Keeping in mind the inflationary behaviour near the bounce, five different scalar field potential functions are explored, and their effect on the equation of state parameter is investigated.
引用
收藏
页数:5
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