中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Phenomenology of quintessino dark matter: Production of next lightest supersymmetric particles

文献类型:期刊论文

作者Bi XJ(毕效军); Wang JX(王建雄); Zhang C(张超); Zhang XM(张新民); Bi, XJ; Wang, JX; Zhang, C; Zhang, XM
刊名PHYSICAL REVIEW D
出版日期2004
卷号70期号:12页码:123512
通讯作者Chinese Acad Sci, Inst High Energy Phys, Beijing 100039, Peoples R China
英文摘要In the model of quintessino as the dark matter particle, the dark matter and dark energy are unified in one superfield, where the dynamics of the Quintessence drives the Universe acceleration and its superpartner, quintessino, makes up the dark matter of the Universe. This scenario predicts the existence of long-lived tau as the next lightest supersymmetric particle. In this paper we study the possibility of detecting tau produced by the high energy cosmic neutrinos interacting with the earth matter. By a detailed calculation we find that the event rate is one to several hundred per year at a detector with an effective area of 1 km(2). The study in this paper can be also applied to models of gravitino or axino dark matter particles.
学科主题Astronomy & Astrophysics; Physics
类目[WOS]Astronomy & Astrophysics ; Physics, Particles & Fields
研究领域[WOS]Astronomy & Astrophysics ; Physics
原文出处SCI
语种英语
WOS记录号WOS:000226054800029
源URL[http://ir.ihep.ac.cn/handle/311005/240979]  
专题高能物理研究所_粒子天体物理中心
作者单位中国科学院高能物理研究所
推荐引用方式
GB/T 7714
Bi XJ,Wang JX,Zhang C,et al. Phenomenology of quintessino dark matter: Production of next lightest supersymmetric particles[J]. PHYSICAL REVIEW D,2004,70(12):123512.
APA 毕效军.,王建雄.,张超.,张新民.,Bi, XJ.,...&Zhang, XM.(2004).Phenomenology of quintessino dark matter: Production of next lightest supersymmetric particles.PHYSICAL REVIEW D,70(12),123512.
MLA 毕效军,et al."Phenomenology of quintessino dark matter: Production of next lightest supersymmetric particles".PHYSICAL REVIEW D 70.12(2004):123512.

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来源:高能物理研究所

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