Possibility of 8B solar neutrino detection via 19F inverse beta-decay reactions

Details Possibility of 8B solar neutrino detection via 19F inverse beta-decay reactions Possibility of 8B solar neutrino detection via 19F inverse beta-decay reactions

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995phla..205....9b&link_type=abstract

Physics Letters A, Volume 205, Issue 1, p. 9-13.

Physics

Scientific paper

A method to detect 8B solar neutrinos is proposed using the charge current reaction νe 19F with a hexafluorobenzene scintillation detector. The main advantage of the detector is the possibility of identifying neutrino events by a delayed coincidence with the β+ decay of 19Ne (T1/(2) = 17 s). Because of this the detector is potentially sensitive to neutrinos with an energy as low as 5 MeV. An additional advantage of the detector is the ability to select unambiguously the electron neutrino component of the burst from a stellar gravitational collapse.

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