Indirect search for neutralino dark matter with high energy neutrinos

被引：94

作者：

Barger, V

Halzen, F

Hooper, D

Kao, C

机构：

[1] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA

[2] Univ Oklahoma, Dept Phys & Astron, Norman, OK 73019 USA

来源：

PHYSICAL REVIEW D | 2002年 / 65卷 / 07期

关键词：

D O I：

10.1103/PhysRevD.65.075022

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We investigate the prospects of indirect searches for supersymmetric neutralino dark matter. Relic neutralinos gravitationally accumulate in the Sun and their annihilations produce high energy neutrinos. Muon neutrinos of this origin can be seen in large detectors such as AMANDA, IceCube, and ANTARES. We evaluate the relic density and the detection rate in several models-the minimal supersymmetric model, minimal supergravity, and supergravity with nonuniversal Higgs boson masses at the grand unification scale. We make realistic estimates for the indirect detection rates including effects of the muon detection threshold, quark hadronization, and solar absorption. We find good prospects for detection of neutralinos with mass above 200 GeV.

引用

页码：750221 / 7502215

页数：15

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