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

页码：117 / 121

页数：5

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