Dark matter asymmetry in supersymmetric Dirac leptogenesis

被引:14
|
作者
Choi, Ki-Young [1 ,2 ]
Chun, Eung Jin [3 ]
Shin, Chang Sub [1 ]
机构
[1] Asia Pacific Ctr Theoret Phys, Pohang 790784, Gyeongbuk, South Korea
[2] POSTECH, Dept Phys, Pohang 790784, Gyeongbuk, South Korea
[3] Korea Inst Adv Study, Seoul 130722, South Korea
基金
新加坡国家研究基金会;
关键词
D O I
10.1016/j.physletb.2013.04.020
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss asymmetric or symmetric dark matter candidate in the supersymmetric Dirac leptogenesis scenario. By introducing a singlet superfield coupling to right-handed neutrinos, the overabundance problem of dark matter can be evaded and various possibilities for dark matter candidate arise. If the singlino is the lightest supersymmetric particle (LSP), it becomes naturally asymmetric dark matter. On the other hand, the right-handed sneutrino is a symmetric dark matter candidate whose relic density can be determined by the usual thermal freeze-out process. The conventional neutralino or gravitino LSP can be also a dark matter candidate as its non-thermal production from the right-handed sneutrino can be controlled appropriately. In our scenario, the late-decay of heavy supersymmetric particles mainly produces the right-handed sneutrino and neutrino which is harmless to the standard prediction of the Big-Bang Nucleosynthesis. (c) 2013 Elsevier B.V. All rights reserved.
引用
收藏
页码:90 / 94
页数:5
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