Extended quintessence and its late-time domination

被引:50
作者
Chiba, T [1 ]
机构
[1] Kyoto Univ, Dept Phys, Kyoto 6068502, Japan
来源
PHYSICAL REVIEW D | 2001年 / 64卷 / 10期
关键词
D O I
10.1103/PhysRevD.64.103503
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Various astronomical observations point towards evidence of dark energy. One of the most mysterious problems is the coincidence problem: why dark energy has become dominant only recently. We present a scenario based on extended quintessence models to explain the late-time domination of dark energy without a severe fine-tuning of the initial conditions and model parameters.
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页数:4
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