A heavy water detector to resolve the solar neutrino problem

Details A heavy water detector to resolve the solar neutrino problem A heavy water detector to resolve the solar neutrino problem

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987phlb..194..321a&link_type=abstract

Physics Letters B, Volume 194, Issue 2, p. 321-325.

Physics

76

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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