Directional Detection of Galactic Dark Matter

被引：1
|
作者：
Mayet, F. [1 ]
Billard, J. [1 ]
Santos, D. [1 ]
机构：
[1] Univ Grenoble 1, CNRS, LPSC, IN2P3,Inst Polytech Grenoble, Grenoble, France
来源：
SOURCES AND DETECTION OF DARK MATTER AND DARK ENERGY IN THE UNIVERSE | 2013年 / 148卷
关键词：
D O I：
10.1007/978-94-007-7241-0_18
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Directional detection is a promising Dark Matter search strategy. Taking advantage on the rotation of the Solar system around the galactic center through the Dark Matter halo, it allows to show a direction dependence of WIMP events that may be a powerful tool to identify genuine WIMP events as such. Directional detection strategy requires the simultaneous measurement of the energy and the 3D track of low energy recoils, which is a common challenge for all current projects of directional detectors.
引用
收藏
页码：117 / 121
页数：5
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