翻訳と辞書
Words near each other
・ Homesick and Happy to Be Here
・ Homesick for St. Pauli
・ Homesick for You
・ Homesick Future
・ Homesick Heroes
・ Homesick James
・ Homesickness
・ Homesite of John O. Meusebach
・ Homesongs
・ Homesourcing
・ Homespun
・ Homespun (band)
・ Homespun (Winchester, Virginia)
・ Homespun Records
・ Homestake
Homestake experiment
・ Homestake Mine
・ Homestake Mine (Nevada)
・ Homestake Mine (South Dakota)
・ Homestake Mining Company
・ Homestake Pass
・ Homestall Farm
・ Homestar Runner
・ Homestay
・ Homestead
・ Homestead (buildings)
・ Homestead (meteorite)
・ Homestead (small African settlement)
・ Homestead (unit)
・ Homestead Act of 1860


Dictionary Lists
翻訳と辞書 辞書検索 [ 開発暫定版 ]
スポンサード リンク

Homestake experiment : ウィキペディア英語版
Homestake experiment
The Homestake experiment (sometimes referred to as the Davis experiment) was an experiment headed by astrophysicists Raymond Davis, Jr. and John N. Bahcall in the late 1960s. Its purpose was to collect and count neutrinos emitted by nuclear fusion taking place in the Sun. Bahcall did the theoretical calculations and Davis designed the experiment. After Bahcall calculated the rate at which the detector should capture neutrinos, Davis's experiment turned up only one third of this figure. The experiment was the first to successfully detect and count solar neutrinos, and the discrepancy in results essentially created the solar neutrino problem. The experiment operated continuously from 1970 until 1994. The University of Pennsylvania took it over in 1984. The discrepancy between the predicted and measured rates of neutrino detection was later found to be due to neutrino "flavour" oscillations.
==Methodology==
The experiment took place in the Homestake Gold Mine in Lead, South Dakota. Davis placed 1,478 meters (4,850 feet) underground a 380 cubic meter (100,000 gallon) tank of perchloroethylene, a common dry-cleaning fluid. A big target deep underground was needed to prevent interference from cosmic rays, taking into account the very small probability of a successful neutrino capture, and, therefore, very low effect rate even with the huge mass of the target. Perchloroethylene was chosen because it is rich in chlorine. Upon interaction with an electron neutrino, a chlorine-37 atom transforms into a radioactive isotope of argon-37, which can then be extracted and counted. The reaction of neutrino capture is
:\mathrmAr + e^-.}
The reaction threshold is 0.814 MeV, i.e. the neutrino should have at least this energy to be captured by the chlorine-37 nucleus.
Every few weeks, Davis bubbled helium through the tank to collect the argon that had formed. A small (few cubic cm) gas counter was filled by the collected few tens atoms of argon-37 (together with the stable argon) to detect its decays. In such way, Davis was able to determine how many neutrinos had been captured.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
ウィキペディアで「Homestake experiment」の詳細全文を読む



スポンサード リンク
翻訳と辞書 : 翻訳のためのインターネットリソース

Copyright(C) kotoba.ne.jp 1997-2016. All Rights Reserved.