Particle dark matter and solar axion searches with a small germanium detector at the Canfranc Underground Laboratory

被引:82
作者
Morales, A [1 ]
Avignone, FT
Brodzinski, RL
Cebrián, S
García, E
González, D
Irastorza, IG
Miley, HS
Morales, J
de Solórzano, AO
Puimedón, J
Reeves, JH
Sarsa, ML
Scopel, S
Villar, JA
机构
[1] Univ Zaragoza, Lab Nucl & High Energy Phys, Zaragoza 50009, Spain
[2] Univ S Carolina, Columbia, SC 29208 USA
[3] Pacific NW Natl Lab, Richland, WA 99352 USA
基金
美国国家科学基金会;
关键词
dark matter; underground detectors; weakly interacting massive particles; axions;
D O I
10.1016/S0927-6505(01)00117-7
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A small, natural abundance, germanium detector (COSME) has been operating recently at the Canfranc Underground Laboratory (Spanish Pyrenees) in improved conditions of shielding and overburden with respect to a previous operation of the same detector (Nucl. Instrum. Meth. A 321 (1992) 410; Phys. Rev. D 51 (1995) 1458). An exposure of 72.7 kg day in these conditions has at present a background improvement of about one order of magnitude compared to the former operation of the detector. These new data have been applied to a direct search for weakly interacting massive particles (WIMPs) and solar axions. New WIMP exclusion plots improving the current bounds for low masses are reported. The paper also presents a limit on the axion-photon coupling obtained from the analysis of the data looking for a Primakoff axion-to-photon conversion and Bragg scattering inside the crystal. (C) 2002 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:325 / 332
页数:8
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