Development of γ-ray detectors for 16O(p,p'γ) experiment

T. Mori; T. Izumi; I. Ou; T. Yano; M. Sakuda; A. Tamii; T. Suzuki; M. Yosoi

doi:10.1063/1.4763450

Development of γ-ray detectors for ¹⁶O(p,p'γ) experiment

T. Mori, T. Izumi, I. Ou, T. Yano, M. Sakuda, A. Tamii, T. Suzuki, M. Yosoi

Graduate School of Natural Science and Technology

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

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	Origin of Matter and Evolution of Galaxies 2011
Pages	451-453
Number of pages	3
DOIs	https://doi.org/10.1063/1.4763450
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

Publication series

Name	AIP Conference Proceedings
Volume	1484
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

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

Keywords

Supernova neutrinos
γ-ray spectra in O

ASJC Scopus subject areas

Physics and Astronomy(all)

Access to Document

10.1063/1.4763450

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Cite this

Mori, T, Izumi, T, Ou, I, Yano, T, Sakuda, M, Tamii, A, Suzuki, T & Yosoi, M 2012, Development of γ-ray detectors for ¹⁶O(p,p'γ) experiment. in Origin of Matter and Evolution of Galaxies 2011. AIP Conference Proceedings, vol. 1484, pp. 451-453, International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011, Wako, Japan, 11/14/11. https://doi.org/10.1063/1.4763450

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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.",

keywords = "Supernova neutrinos, γ-ray spectra in O",

author = "T. Mori and T. Izumi and I. Ou and T. Yano and M. Sakuda and A. Tamii and T. Suzuki and M. Yosoi",

note = "Copyright: Copyright 2013 Elsevier B.V., All rights reserved.; International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011 ; Conference date: 14-11-2011 Through 17-11-2011",

year = "2012",

doi = "10.1063/1.4763450",

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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

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