Homestake experiment 2026-10-18
The Homestake experiment, led by Raymond Davis Jr., used electron neutrino capture on chlorine to produce argon subject to radioactive decay. The 1968 paper reported an upper limit, rather than a resolved positive signal.[ref]
Search for Neutrinos from the Sun by Raymond Davis Jr. and others. Abstract: chlorine reaction and upper-limit result
The underground target contained tetrachloroethylene. Circulated helium swept out argon, which was trapped on cooled charcoal, purified, and put into tiny proportional counters. Electron capture back to chlorine supplies the delayed readout. Added stable argon checked extraction recovery; background counting checked spurious pulses. The capture threshold is and the product's half-life is about 35 days. The chemical extraction retains neither the original neutrino's arrival time nor its direction.[ref]
Nobel Lecture: A half-century with solar neutrinos by Raymond Davis Jr.. pp. 986, 988–991; Figs. 9–14
The reaction selects electron neutrinos, and its threshold excludes the lowest-energy part of the solar neutrino spectrum. A low count alone cannot distinguish a low source neutrino flux, a changed neutrino flavor mixture, or an underestimated loss in extraction or counting. This is why chemical recovery tests and an independent water Cherenkov neutrino reconstruction are scientifically valuable.
How can a detector establish that an unseen particle changes identity? The Super-Kamiokande atmospheric-neutrino experiment compares different travel paths; the Sudbury Neutrino Observatory compares different interaction channels. Both infer neutrino flavor from reaction products and calibrated responses. Their complementarity connects particle detection to neutrino oscillation, neutrino mass and neutrino astronomy.
Takaaki Kajita and Arthur B. McDonald shared the 2015 physics Nobel Prize. These were collaboration achievements: Yoichiro Suzuki's Super-Kamiokande work included the solar neutrino analysis, and George Ewan helped establish and lead the Sudbury Neutrino Observatory.[ref]
ICRR’s Takaaki Kajita to share Breakthrough Prize in Fundamental Physics by Institute for Cosmic Ray Research, University of Tokyo. Research contributions of Kajita and Suzuki; shared 2015 prize
[ref]https://www.queensu.ca/gazette/stories/queen-s-remembers-professor-emeritus-george-ewan/. 17 December 2020: founding and joint leadership of SNO
The older Kamiokande account explains water Cherenkov neutrino reconstruction; Raymond Davis Jr.'s Homestake experiment explains why a deficit in an electron neutrino channel alone leaves a source-versus-propagation ambiguity. Complementary channels can break that ambiguity.
Nobel Prize in Physics in 2002 2026-10-18
One quarter each went to Raymond Davis Jr. and Masatoshi Koshiba for pioneering astrophysics through detection of cosmic neutrinos. One half went to Riccardo Giacconi for pioneering astrophysics leading to the discovery of cosmic X-ray sources.[ref]
The Nobel Prize in Physics 2002 by Nobel Prize Outreach. Individual official 2002 summary: Davis and Koshiba one quarter each for cosmic neutrinos; Giacconi one half for cosmic X-ray sources.
Raymond Davis Jr. 2026-10-18
Portrait of Raymond Davis Jr.
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