SEARCHING FOR TEV DARK MATTER BY ATMOSPHERIC CERENKOV TECHNIQUES

被引：50

作者：

URBAN, M

BOUQUET, A

DEGRANGE, B

FLEURY, P

KAPLAN, J

MELCHIOR, AL

PARE, E

机构：

[1] UNIV PARIS 06,PHYS THEOR & HAUTES ENERGIES LAB,F-75251 PARIS 05,FRANCE

[2] UNIV PARIS 07,F-75251 PARIS 05,FRANCE

来源：

PHYSICS LETTERS B | 1992年 / 293卷 / 1-2期

关键词：

D O I：

10.1016/0370-2693(92)91494-T

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

There is a growing interest in the possibility that dark matter could be formed of weakly interacting particles with a mass in the 1 00 GeV-2 TeV range, and supersymmetric particles are favorite candidates. If they constitute the dark halo of our Galaxy, their mutual annihilations produce energetic gamma rays that could be detected using existing atmospheric Cerenkov techniques.

引用

页码：149 / 156

页数：8

共 39 条

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