Models of Dark Energy

被引：7
作者：
Copeland, Edmund J. [1 ]
机构：
[1] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England
来源：
INVISIBLE UNIVERSE INTERNATIONAL CONFERENCE | 2010年 / 1241卷
关键词：
Dark energy; Cosmology; SMALL COSMOLOGICAL CONSTANT; GRAVITY; QUINTESSENCE; LAMBDA;
D O I：
10.1063/1.3462965
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
I briefly review models of dark energy. These include models of a cosmological constant arising in string theory, dynamical models where a scalar field may be responsible for the observed late time acceleration through to the possibility that we are not fully in control of the gravity sector and the acceleration may be some manifestation of modified gravity. All cases require some degree of fine tuning for the models to be compatible with observation.
引用
收藏
页码：125 / 131
页数：7
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