Neutralino dark matter searches with neutrino telescopes: AMANDA results and IceCube prospects

被引：7
|
作者：
Hubert, D. [1 ]
机构：
[1] Vrije Univ Brussel, Dienst ELEM, B-1050 Brussels, Belgium
来源：
NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS | 2007年 / 173卷
关键词：
D O I：
10.1016/j.nuclphysbps.2007.08.058
中图分类号：
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号：
摘要：
If non-baryonic dark matter exists in the form of neutralinos, they may accumulate in massive celestial bodies leading to a neutrino flux from the decay products of neutralino pair annihilation. Data taken with high energy neutrino telescopes can be used in a search for this indirect dark matter signal. We will present current results from searches for neutralinos accumulated in the Earth and the Sun, using AMANDA data from 1997-1999 and 2001 respectively. We also discuss future improvements for higher statistics AMANDA data samples acquired during recent years and the indirect dark matter detection prospects for the 1 km 3 IceCube detector, currently under construction at the South Pole.
引用
收藏
页码：87 / 90
页数：4
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