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Solar Neutrino Research
Basic research on solar neutrinos has a long history in the Brookhaven Chemistry Department. This group initiated and operated the pioneering experiments that first uncovered the famous solar neutrino deficit using chemical detection of nuclear transformations induced by solar neutrinos using 615 tons of C2Cl4, and later participated in the GALLEX solar neutrino experiments in Gran Sasso, Italy where 30 tons of Gallium comprised the neutrino detector. The pioneering experiments conducted in the Homestake Mine, Lead, South Dakota, led to the awarding of the 2002 Nobel Prize in Physics to Raymond Davis, Jr., the founder of this group. Currently, the Solar Neutrino Research Group is a participant in the very successful solar neutrino detector, the Solar Neutrino Observatory (SNO) in Sudbury, Ontario. The neutrino detection medium in SNO is 1000-metric-tons of D2O, which is valued at ~US$ 300 Million. The Solar Neutrino Group is also actively involved in R&D on proposed future neutrino experiments: (1) in the real-time detection of the lowest energy neutrinos from the Sun, in the Low Energy Neutrino Spectroscopy (LENS-Sol) Collaboration; (2) in the Brookhaven Physics Department project to develop a long-baseline muon-neutrino oscillation experiment, using an intense wide-band beam (~1-7 GeV) of muon-neutrinos from the Alternating Gradient Synchrotron to be directed to an underground laboratory ~2000 km from BNL;(3) in two different international "Theta-13" collaborations that are planning future high-precision experiments at the ~1% level, to measure oscillation patterns of antineutrinos emanating from nuclear power reactors. For further information, see also here and here. The Solar Neutrino Research Group is supported by the the Low Energy Nuclear Physics Program of the Office of Nuclear Physics of the Office of Science under contract No. DE-AC02-98CH10886 with the U.S. Department of Energy.
Last Modified: January 31, 2008 |