Physics – Nuclear Physics
Scientific paper
Aug 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1269..418m&link_type=abstract
THE 10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: OMEG-2010. AIP Conference Proceedings, Volume 1
Physics
Nuclear Physics
Neutral Currents, Supernovae, Gamma-Rays, Nuclear Spin, Neutral Currents, Supernovae, X- And Gamma-Ray Sources, Mirrors, Gratings, And Detectors, Spin, Parity, And Isobaric Spin
Scientific paper
The γ-ray production in neutral-current (NC) neutrino-oxygen interaction is very important to the detection of neutrinos from supernova explosion in a neutrino experiment using water target like Super-K, since those γ-rays can become extra signals or unexpected background in the energy region from 5 MeV to 30 MeV. We discuss a possible experiment to measure γ-rays in 16O(p, p') and 16O(3He, t) reactions at Research Center for Nuclear Physics (RCNP, Osaka). Such measurements should provide good information on the γ-ray emission spectra in neutrino-oxygen reactions.
Mori Tadashi
Nakahata Masayuki
Sakuda Makoto
Tamii Atsushi
Toki Hiroshi
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