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The Homestake experiment (sometimes referred to as the Davis experiment or Solar Neutrino Experiment and in original literature called Brookhaven Solar Neutrino Experiment or Brookhaven 37 Cl (Chlorine) Experiment) [1] was an experiment headed by astrophysicists Raymond Davis, Jr. and John N. Bahcall in the late 1960s.
The Sanford Underground Research Facility (SURF), or Sanford Lab, is an underground laboratory in Lead, South Dakota. The deepest underground laboratory in the United States, it houses multiple experiments in areas such as dark matter and neutrino physics research, biology, geology and engineering. There are currently 28 active research ...
Homestake chlorine experiment S ν e: 37 Cl + ν e → 37 Ar * + e − 37 Ar * → 37 Cl + e + + ν e: CC C 2 Cl 4 (615 t) Radiochemical: 814 keV Homestake Mine, South Dakota: 1967–1998 HOMESTAKE–IODINE Homestake iodine experiment S ν e: ν + e − → ν + e − ν e + 127 I → 127 Xe + e −: ES CC NaI in water Radiochemical: 789 keV ...
Raymond Davis Jr. (October 14, 1914 – May 31, 2006) was an American chemist and physicist.He is best known as the leader of the Homestake experiment in the 1960s-1980s, which was the first experiment to detect neutrinos emitted from the Sun; for this he shared the 2002 Nobel Prize in Physics.
The Homestake Mine is famous in scientific circles because of the work of a deep underground laboratory that was established there in the mid-1960s. This was the site where the solar neutrino problem was first discovered, in what is known as the Homestake Experiment.
"We can trust these results," Glavin said. Bennu's icy parent body, perhaps about 60 miles (100 km) in diameter, appears to have formed in the outer solar system and was later destroyed, possibly ...
The January 9 report only shared results for lead, cadmium, BPA, and BPS testing. ... For the study, an independent certified laboratory ran nearly 36,000 tests on 258 different contaminants.
The Sudbury Neutrino Observatory (SNO), a 2,100 m (6,900 ft) underground observatory in Sudbury, Canada, is the other site where neutrino oscillation research was taking place in the late 1990s and early 2000s. The results from experiments at this observatory along with those at Super-Kamiokande are what helped solve the solar neutrino problem.