Abstract
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.
| Original language | English |
|---|---|
| Title of host publication | AIP Conference Proceedings |
| Pages | 451-453 |
| Number of pages | 3 |
| Volume | 1484 |
| DOIs | |
| Publication status | Published - 2012 |
| Event | International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011 - Wako, Japan Duration: Nov 14 2011 → Nov 17 2011 |
Other
| Other | International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011 |
|---|---|
| Country | Japan |
| City | Wako |
| Period | 11/14/11 → 11/17/11 |
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Keywords
- γ-ray spectra in O
- Supernova neutrinos
ASJC Scopus subject areas
- Physics and Astronomy(all)
Cite this
Development of γ-ray detectors for 16O(p,p'γ) experiment. / Mori, T.; Izumi, T.; Ou, I.; Yano, T.; Sakuda, Makoto; Tamii, A.; Suzuki, T.; Yosoi, M.
AIP Conference Proceedings. Vol. 1484 2012. p. 451-453.Research output: Chapter in Book/Report/Conference proceeding › Conference contribution
}
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, Makoto
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 - γ-ray spectra in O
KW - Supernova neutrinos
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
VL - 1484
SP - 451
EP - 453
BT - AIP Conference Proceedings
ER -