Indirect detection of dark matter weakly interacting massive particles in a liquid argon time projection chamber

被引：0
|
作者：
Bueno, A [1 ]
Cid, R
Navas-Concha, S
Hooper, D
Weiler, TJ
机构：
[1] Univ Granada, Dept Fis Teor & Cosmos, Granada, Spain
[2] Univ Granada, CAFPE, Granada, Spain
[3] Univ Oxford, Dept Astrophys, Oxford OX1 3RH, England
[4] Vanderbilt Univ, Dept Phys & Astron, Nashville, TN 37235 USA
来源：
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2005年 / 01期
关键词：
solar and atmospheric neutrinos; cosmology of theories beyond the SM;
D O I：
10.1008/1475-7516/2005/01/001
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We assess the prospects for indirect detection of weakly interacting massive particles using a large liquid argon TPC detector. Signal events will consist of energetic electron (anti) neutrinos coming from the decay of tau leptons and b quarks produced in WIMP annihilation in the core of the Sun. Background contamination from atmospheric neutrinos is expected to be low, thanks to the superb angular resolution and particle identification capabilities provided by the experimental set-up considered. We evaluate the event rates predicted for an annihilating WIMP as a function of its elastic scattering cross section for nucleons. This technique is particularly useful for WIMPs lighter than similar to100 GeV.
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页数：15
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