Fermionic partner of the quintessence field as a candidate for dark matter
被引:19
作者:
Bi, XJ
论文数: 0引用数: 0
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机构:
Chinese Acad Sci, Inst High Energy Phys, Beijing 100039, Peoples R ChinaChinese Acad Sci, Inst High Energy Phys, Beijing 100039, Peoples R China
Bi, XJ
[1
]
Li, MZ
论文数: 0引用数: 0
h-index: 0
机构:
Chinese Acad Sci, Inst High Energy Phys, Beijing 100039, Peoples R ChinaChinese Acad Sci, Inst High Energy Phys, Beijing 100039, Peoples R China
Li, MZ
[1
]
Zhang, XM
论文数: 0引用数: 0
h-index: 0
机构:
Chinese Acad Sci, Inst High Energy Phys, Beijing 100039, Peoples R ChinaChinese Acad Sci, Inst High Energy Phys, Beijing 100039, Peoples R China
Zhang, XM
[1
]
机构:
[1] Chinese Acad Sci, Inst High Energy Phys, Beijing 100039, Peoples R China
来源:
PHYSICAL REVIEW D
|
2004年
/
69卷
/
12期
关键词:
D O I:
10.1103/PhysRevD.69.123521
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
Quintessence is a possible candidate for dark energy. In this paper we study the phenomenologies of the fermionic partner of quintessence, the quintessino. Our results show that, for suitable choices of the model parameters, the quintessino is a good candidate for cold or warm dark matter. In our scenario, the dark energy and dark matter of the Universe are connected in one chiral superfield.