Measurement of the solar electron neutrino flux with the Homestake chlorine detector

被引:1706
作者
Cleveland, BT
Daily, T
Davis, R
Distel, JR
Lande, K
Lee, CK
Wildenhain, PS
Ullman, J
机构
[1] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA
[2] CUNY Herbert H Lehman Coll, Dept Phys & Astron, Bronx, NY 10468 USA
关键词
elementary particles; Sun; interior; particle emission;
D O I
10.1086/305343
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Homestake Solar Neutrino Detector, based on the inverse beta-decay reaction v(e) + Cl-37 --> Ar-37 + e(-), has been measuring the flux of solar neutrinos since 1970. The experiment has operated in a stable manner throughout this time period. All aspects of this detector are reviewed, with particular emphasis on the determination of the extraction and counting efficiencies, the key experimental parameters that are necessary to convert the measured Ar-37 count rate to the solar neutrino production rate. A thorough consideration is also given to the systematics of the detector, including the measurement of the extraction and counting efficiencies and the nonsolar production of Ar-37. Th, combined result of 108 extractions is a solar neutrino-induced Ar-37 production rate of 2.56 +/- 0.16 (statistical) +/- 0.16 (systematic) SNU.
引用
收藏
页码:505 / 526
页数:22
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