Indirect dark matter searches in gamma and cosmic rays

被引：0
|
作者：
Conrad J. [1 ]
Reimer O. [2 ]
机构：
[1] Oskar Klein Center, Physics Department, Stockholm University, Roslagstullsbacken 21, Stockholm
[2] Institute for Astro- and Particle Physics, Innsbruck University, Technikerstrasse 25/8, Innsbruck
来源：
Nature Physics | 2017年 / 13卷 / 3期
关键词：
D O I：
10.1038/nphys4049
中图分类号：
学科分类号：
摘要：
Dark matter candidates such as weakly interacting massive particles are predicted to annihilate or decay into Standard Model particles, leaving behind distinctive signatures in gamma rays, neutrinos, positrons, antiprotons, or even antinuclei. Indirect dark matter searches, and in particular those based on gamma-ray observations and cosmic-ray measurements, could detect such signatures. Here we review the strengths and limitations of this approach and look into the future of indirect dark matter searches. © 2017 Macmillan Publishers Limited.
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页码：224 / 231
页数：7
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