A heavy water detector to resolve the solar neutrino problem

Physics

Scientific paper

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Scientific paper

The observation of the following three reactions: νed-->ppe νxe-->νxe and νxd-->νxpn (where νx is any left- handed neutrino) in a heavy water Čerenkov detector which is being designed, allows the solar 8B ve flux, spectrum and direction to be measured. In addition, the total solar 8Bνc neutrino flux, direction and integral spectrum, independent of neutrino flavor, may be determined to provide several independent methods to resolve the solar neutrino problem.

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