Indirect detection of Dark Matter with the ANTARES Neutrino Telescope

被引：0
|
作者：
Ardid, Miguel [1 ]
机构：
[1] Univ Politecn Valencia, Inst Invest Gestio Integrada Zones Costaneres IGI, C Paranimf 1, Gandia 46730, Spain
来源：
VERY LARGE VOLUME NEUTRINO TELESCOPE (VLVNT-2015) | 2016年 / 116卷
关键词：
D O I：
10.1051/epjconf/201611604002
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
One of the main objectives of the ANTARES neutrino telescope is the search for neutrinos produced in self-annihilation of Dark Matter (DM) particles. The analysis for different sources of DM (Sun, Galactic Center, Earth, ...) or DM models (SUSY, Secluded) will be described and the results presented. The specific advantages of neutrino telescopes in general and of ANTARES in particular will be explained. As an example, the indirect search for DM towards the Sun performed by neutrino telescopes currently leads to more stringent limits on the spin-dependent WIMP-nucleon cross section with respect to existing direct detection experiments.
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页数：5
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