Imaging dark matter with the Pamela experiment

被引：6
|
作者：
Boezio, M. [1 ]
Pearce, M. [2 ]
机构：
[1] INFN Trieste, Via Valerio 2, I-34127 Trieste, Italy
[2] Royal Institute of Technology (KTH), Physics Department Frescati, Frescativägen 24, S-10405 Stockholm, Sweden
来源：
Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment | 2001年 / 471卷 / 1-2期
关键词：
Cosmic rays - Imaging techniques - Orbits - Satellites - Silicon - Spectrometers;
D O I：
10.1016/S0168-9002(01)00997-4
中图分类号：
学科分类号：
摘要：
The search for dark matter is a fundamental issue for astroparticle physics. A satellite-borne experiment ('Pamela') is under construction and will study cosmic rays whilst executing a polar orbit at an altitude of 690 km. The experiment comprises a transition radiation detector; a magnetic spectrometer, incorporating silicon tracking and surrounded by an anti-coincidence shield; an electromagnetic imaging calorimeter and a time-of-flight trigger system. This combination of detectors is particularly apt for the study of the antiproton component of cosmic rays from 100 MeV up to a few 100 GeV and will provide important new information for dark matter searches. © 2001 Elsevier Science B.V. All rights reserved.
引用
收藏
页码：184 / 187
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