TY - GEN
T1 - Development of γ-ray detectors for 16O(p,p'γ) experiment
AU - Mori, T.
AU - Izumi, T.
AU - Ou, I.
AU - Yano, T.
AU - Sakuda, M.
AU - Tamii, A.
AU - Suzuki, T.
AU - Yosoi, M.
PY - 2012
Y1 - 2012
N2 - 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, since those γ rays can become extra signals or unexpected background in the energy region from 5 MeV to 30 MeV. We propose the experiment to measure γ rays in 16O(p,p') reaction at Research Center for Nuclear Physics (RCNP, Osaka) to provide good information on the γ-ray emission spectra in neutrino-oxygen reactions. We present the design of γ-ray detectors (NaI, CsI, HPGe), which will be used in proposed experiment.
AB - 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, since those γ rays can become extra signals or unexpected background in the energy region from 5 MeV to 30 MeV. We propose the experiment to measure γ rays in 16O(p,p') reaction at Research Center for Nuclear Physics (RCNP, Osaka) to provide good information on the γ-ray emission spectra in neutrino-oxygen reactions. We present the design of γ-ray detectors (NaI, CsI, HPGe), which will be used in proposed experiment.
KW - Supernova neutrinos
KW - γ-ray spectra in O
UR - http://www.scopus.com/inward/record.url?scp=84874539509&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84874539509&partnerID=8YFLogxK
U2 - 10.1063/1.4763450
DO - 10.1063/1.4763450
M3 - Conference contribution
AN - SCOPUS:84874539509
SN - 9780735410961
T3 - AIP Conference Proceedings
SP - 451
EP - 453
BT - Origin of Matter and Evolution of Galaxies 2011
T2 - International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011
Y2 - 14 November 2011 through 17 November 2011
ER -