The search for dark matter via gamma rays from astronomical sources using EGRET and GLAST

被引：2
|
作者：
Bloom, ED [1 ]
机构：
[1] Stanford Univ, Stanford Linear Accelerator Ctr, Menlo Pk, CA 94025 USA
来源：
NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS | 2004年 / 134卷
关键词：
D O I：
10.1016/j.nuclphysbps.2004.08.016
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：
EGRET, aboard NASA's CGRO satellite, has made important contributions to establishing Emits on WIMP dark matter in the galaxy. This paper will review these EGRET results. Based on past Emits and theoretical estimates, future potential dark matter results from GLAST are projected.
引用
收藏
页码：103 / 111
页数：9
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