Phenomenology of quintessino dark matter: Production of next lightest supersymmetric particles

被引：16

作者：

Bi, XJ ^{[1
]}

Wang, JX ^{[1
]}

Zhang, C ^{[1
]}

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 / 70卷 / 12期

基金：

中国国家自然科学基金; 中国博士后科学基金;

关键词：

D O I：

10.1103/PhysRevD.70.123512

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

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.

引用

页码：123512 / 1

页数：7

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