Dark matter chaotic inflation in light of BICEP2

被引:15
作者
Mukaida, Kyohei [1 ]
Nakayama, Kazunori [1 ,2 ]
机构
[1] Univ Tokyo, Fac Sci, Dept Phys, Bunkyo Ku, Tokyo 1330033, Japan
[2] Univ Tokyo, Todai Inst Adv Study, Kavli Inst Phys & Math Universe, Kashiwa, Chiba 2778583, Japan
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2014年 / 08期
关键词
inflation; particle physics - cosmology connection; physics of the early universe; cosmology of theories beyond the SM; UNIVERSE; FLATNESS; HORIZON; MODEL;
D O I
10.1088/1475-7516/2014/08/062
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We propose an economical model in which a singlet Z(2)-odd scalar field accounts for the primordial inflation and the present dark matter abundance simultaneously in the light of recent BICEP2 result. Interestingly, the reheating temperature and the thermal dark matter abundance are closely connected by the same interaction between the singlet scalar and the standard model Higgs. In addition, the reheating temperature turns out to be quite high, T-R greater than or similar to 10(12) GeV, and hence the thermal leptogenesis is compatible with this model. Therefore, it can be one of the simplest cosmological scenarios.
引用
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页数:13
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