Search for dark matter with GLAST

被引：1
作者：
Morselli, Aldo
机构：
[1] Ist Nazl Fis Nucl, I-00133 Rome, Italy
[2] Univ Roma Tor Vergata, I-00133 Rome, Italy
来源：
CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS | 2006年 / 6卷
关键词：
instrumentation : detectors; dark matter; GRB;
D O I：
10.1088/1009-9271/6/S1/45
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The detection of gamma-rays, antiprotons and positrons due to pair annihilation of dark matter particles in the Milky Way halo is a viable techniques to search for supersymmetric dark matter candidates. In particular the EGRET team has seen a convincing signal for a strong excess of emission from the Galactic center that has no simple explanation with standard processes. We will review the limits achievable with the experiment GLAST and we will compare this method with the antiproton and positrons experiments.
引用
收藏
页码：349 / 356
页数：8
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