Transient and late time attractor tachyon dark energy: Can we distinguish it from quintessence?

被引:29
|
作者
Ali, Amna [1 ]
Sami, M. [1 ]
Sen, A. A. [1 ]
机构
[1] Jamia Millia Islamia, Ctr Theoret Phys, New Delhi 110025, India
来源
PHYSICAL REVIEW D | 2009年 / 79卷 / 12期
关键词
COSMOLOGICAL CONSTANT; DYNAMICS; COINCIDENCE; UNIVERSE; FIELD;
D O I
10.1103/PhysRevD.79.123501
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The string inspired tachyon field can serve as a candidate of dark energy. Its equation of state parameter w varies from 0 to -1. In the case of tachyon field potential V(phi) -> 0 slower (faster) than 1/phi(2) at infinity, dark energy (dark matter) is a late time attractor. We investigate the tachyon dark energy models under the assumption that w is close to -1. We find that all the models exhibit unique behavior around the present epoch which is exactly the same as that of the thawing quintessence.
引用
收藏
页数:7
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