Detectability of galactic supernova neutrinos coherently scattered on xenon nuclei in XMASS

被引：20

作者：

Abe, K. ^{[1
,4
]}

Hiraide, K. ^{[1
,4
]}

Ichimura, K. ^{[1
,4
]}

Kishimoto, Y. ^{[1
,4
]}

Kobayashi, K. ^{[1
,4
,9
]}

Kobayashi, M. ^{[1
]}

Moriyama, S. ^{[1
,4
]}

Nakagawa, K. ^{[1
]}

Nakahata, M. ^{[1
,4
]}

Norita, T. ^{[1
]}

Ogawa, H. ^{[1
,4
]}

Sekiya, H. ^{[1
,4
]}

Takachio, O. ^{[1
]}

Takeda, A. ^{[1
,4
]}

Yamashita, M. ^{[1
,4
]}

Yang, B. S. ^{[1
,4
]}

Kim, N. Y. ^{[2
]}

Kim, Y. D. ^{[2
]}

Tasaka, S. ^{[1
,3
]}

Liu, J. ^{[4
]}

Martens, K. ^{[4
]}

Suzuki, Y. ^{[4
]}

Fujita, R. ^{[6
]}

Hosokawa, K.

Miuchi, K. ^{[6
]}

Oka, N. ^{[6
]}

Onishi, Y. ^{[6
]}

Takeuchi, Y. ^{[4
,6
]}

Kim, Y. H. ^{[2
,7
]}

Lee, J. S. ^{[7
]}

Lee, K. B. ^{[7
]}

Lee, M. K. ^{[7
]}

Fukuda, Y. ^{[8
]}

Itow, Y. ^{[5
,9
]}

Kegasa, R. ^{[9
]}

Kobayashi, K. ^{[1
,4
,9
]}

Masuda, K. ^{[9
]}

Takiya, H. ^{[9
]}

Uchida, H. ^{[9
]}

Nishijima, K. ^{[10
]}

Fujii, K. ^{[11
]}

Murayama, I. ^{[11
]}

Nakamura, S. ^{[11
]}

机构：

[1] Univ Tokyo, Inst Cosm Ray Res, Kamioka Observ, Gifu 5061205, Japan

[2] Ctr Underground Phys, Inst Basic Sci, 70 Yuseong Daero 1689 Gil, Daejeon 305811, South Korea

[3] Gifu Univ, Informat & Multimedia Ctr, Gifu 5011193, Japan

[4] Univ Tokyo, Kavli Inst Phys & Math Universe WPI, Kashiwa, Chiba 2778582, Japan

[5] Nagoya Univ, Kobayashi Maskawa Inst Origin Particles & Univers, Chikusa Ku, Furo Cho, Nagoya, Aichi 4648602, Japan

[6] Kobe Univ, Dept Phys, Kobe, Hyogo 6578501, Japan

[7] Korea Res Inst Stand & Sci, Daejeon 305340, South Korea

[8] Miyagi Univ Educ, Dept Phys, Sendai, Miyagi 9800845, Japan

[9] Nagoya Univ, Inst Space Earth Environm Res, Nagoya, Aichi 4648602, Japan

[10] Tokai Univ, Dept Phys, Hiratsuka, Kanagawa 2591292, Japan

[11] Yokohama Natl Univ, Fac Engn, Dept Phys, Yokohama, Kanagawa 2408501, Japan

[12] Univ South Dakota, Dept Phys, Vermillion, SD 57069 USA

来源：

ASTROPARTICLE PHYSICS | 2017年 / 89卷

基金：

新加坡国家研究基金会;

关键词：

Supernova; Neutrino; Coherent scattering; Liquid xenon; CORE-COLLAPSE SUPERNOVAE; WEAK NEUTRAL-CURRENT; EXPLOSION MECHANISM; SEARCH; ELECTRON; DETECTOR; BURST;

D O I：

10.1016/j.astropartphys.2017.01.006

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The coherent elastic neutrino-nucleus scattering (CEvNS) plays a crucial role at the final evolution of stars. The detection of it would be of importance in astroparticle physics. Among all available neutrino sources, galactic supernovae give the highest neutrino flux in the MeV range. Among all liquid xenon dark matter experiments, XMASS has the largest sensitive volume and light yield. The possibility to detect galactic supernova via the CEvNS-process on xenon nuclei in the current XMASS detector was investigated. The total number of events integrated in about 18 s after the explosion of a supernova 10 kpc away from the Earth was expected to be from 3.5 to 21.1, depending on the supernova model used to predict the neutrino flux, while the number of background events in the same time window was measured to be negligible. All lead to very high possibility to detect CEvNS experimentally for the first time utilizing the combination of galactic supernovae and the XMASS detector. In case of a supernova explosion as close as Betelgeuse, the total observable events can be more than similar to 10(4), making it possible to distinguish different supernova models by examining the evolution of neutrino event rate in XMASS. (C) 2017 Elsevier B.V. All rights reserved.

引用

页码：51 / 56

页数：6

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