Experimental search for solar axions via coherent Primakoff conversion in a germanium spectrometer

被引:94
作者
Avignone, FT [1 ]
Abriola, D
Brodzinski, RL
Collar, JI
Creswick, RJ
DiGregorio, DE
Farach, HA
Gattone, AO
Guérard, CK
Hasenbalg, F
Huck, H
Miley, HS
Morales, A
Morales, J
Nussinov, S
de Solórzano, AO
Reeves, JH
Villar, JA
Zioutas, K
机构
[1] Univ S Carolina, Dept Phys & Astron, Columbia, SC 29208 USA
[2] CNEA, TANDAR Lab, Dept Phys, Buenos Aires, DF, Argentina
[3] Pacific NW Lab, Richland, WA 99352 USA
[4] CERN, CH-1211 Geneva 23, Switzerland
[5] Univ Zaragoza, Lab Fis Nucl & Altas Energias, Zaragoza, Spain
[6] Tel Aviv Univ, Dept Phys, IL-69978 Tel Aviv, Israel
[7] Univ Thessaloniki, Dept Phys, GR-54006 Thessaloniki, Greece
关键词
D O I
10.1103/PhysRevLett.81.5068
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Results are reported of an experimental search for the unique, rapidly varying temporal pattern of solar axions coherently converting into photons via the Primakoff effect in a single crystal germanium detector when axions are incident at a Bragg angle with a crystalline plane. The analysis of 1.94 kg yr of data from the I kg DEMOS detector in Sierra Grande, Argentina, yields a new laboratory bound by an axion-photon coupling of g(a gamma gamma) < 2.7 x 10(-9) GeV-1, independent of axion mass up to similar to 1 keV. [S0031-9007(98)07812-0].
引用
收藏
页码:5068 / 5071
页数:4
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