Search for Solar Flare Neutrinos with the KamLAND Detector

被引：2

作者：

Abe, S. ^{[1
]}

Asami, S. ^{[1
]}

Gando, A. ^{[1
]}

Gando, Y. ^{[1
]}

Gima, T. ^{[1
]}

Goto, A. ^{[1
]}

Hachiya, T. ^{[1
]}

Hata, K. ^{[1
]}

Hayashida, S. ^{[1
,23
]}

Hosokawa, K. ^{[1
,27
]}

Ichimura, K. ^{[1
]}

Ieki, S. ^{[1
]}

Ikeda, H. ^{[1
]}

Inoue, K. ^{[1
,2
]}

Ishidoshiro, K. ^{[1
]}

Kamei, Y. ^{[1
]}

Kawada, N. ^{[1
]}

Kishimoto, Y. ^{[1
,2
]}

Kinoshita, T. ^{[1
]}

Koga, M. ^{[1
,2
]}

Maemura, N. ^{[1
]}

Mitsui, T. ^{[1
]}

Miyake, H. ^{[1
]}

Nakamura, K. ^{[1
]}

Nakamura, R. ^{[1
]}

Ozaki, H. ^{[1
,3
]}

Sakai, T. ^{[1
]}

Sambonsugi, H. ^{[1
]}

Shimizu, I ^{[1
]}

Shirai, J. ^{[1
]}

Shiraishi, K. ^{[1
]}

Suzuki, A. ^{[1
]}

Suzuki, Y. ^{[1
]}

Takeuchi, A. ^{[1
]}

Tamae, K. ^{[1
]}

Ueshima, K. ^{[1
,24
]}

Wada, Y. ^{[1
]}

Watanabe, H. ^{[1
]}

Yoshida, Y. ^{[1
]}

Obara, S. ^{[4
]}

Ichikawa, A. K. ^{[5
]}

Kozlov, A. ^{[2
,25
]}

Chernyak, D. ^{[2
,26
]}

Takemoto, Y. ^{[6
,27
]}

Yoshida, S. ^{[6
]}

Umehara, S. ^{[7
]}

Fushimi, K. ^{[8
]}

Nakamura, K. Z. ^{[9
]}

Yoshida, M. ^{[9
]}

Berger, B. E. ^{[2
,10
]}

机构：

[1] Tohoku Univ, Res Ctr Neutrino Sci, Sendai, Miyagi 9808578, Japan

[2] Univ Tokyo, Inst Phys & Math Universe, Kashiwa, Chiba 2778568, Japan

[3] Tohoku Univ, Grad Program Phys Universe, Sendai, Miyagi 9808578, Japan

[4] Tohoku Univ, Frontier Res Inst Interdisciplinary Sci, Sendai, Miyagi 9808578, Japan

[5] Tohoku Univ, Dept Phys, Sendai, Miyagi 9808578, Japan

[6] Osaka Univ, Grad Sch Sci, Toyonaka, Osaka 5600043, Japan

[7] Osaka Univ, Res Ctr Nucl Phys RCNP, Ibaraki, Osaka 5670047, Japan

[8] Tokushima Univ, Grad Sch Adv Technol & Sci, Tokushima 7708506, Japan

[9] Kyoto Univ, Dept Phys, Kyoto 6068502, Japan

[10] Lawrence Berkeley Natl Lab, Nucl Sci Div, Berkeley, CA 94720 USA

[11] Univ Hawaii Manoa, Dept Phys & Astron, Honolulu, HI 96822 USA

[12] MIT, 77 Massachusetts Ave, Cambridge, MA 02139 USA

[13] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA

[14] Triangle Univ Nucl Lab, Durham, NC 27708 USA

[15] Univ N Carolina, Chapel Hill, NC 27599 USA

[16] North Carolina Cent Univ, Durham, NC 27701 USA

[17] Duke Univ, Phys Dept, Durham, NC 27705 USA

[18] Univ Washington, Ctr Expt Nucl Phys & Astrophys, Seattle, WA 98195 USA

[19] Nikhef, Sci Pk, Amsterdam, Netherlands

[20] Univ Amsterdam, Sci Pk, Amsterdam, Netherlands

[21] Boston Univ, Boston, MA 02215 USA

[22] Virginia Polytech Inst & State Univ, Ctr Neutrino Phys, Blacksburg, VA 24061 USA

[23] Imperial Coll London, Dept Phys, Blackett Lab, London SW7 2AZ, England

[24] Natl Inst Quantum & Radiol Sci & Technol QST, Mikazuki, Hyogo 6795148, Japan

[25] Natl Res Nucl Univ MEPhI, Moscow Engn Phys Inst, Moscow 115409, Russia

[26] Univ Alabama, Dept Phys & Astron, Tuscaloosa, AL 35487 USA

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

来源：

ASTROPHYSICAL JOURNAL | 2022年 / 924卷 / 02期

基金：

荷兰研究理事会; 美国国家科学基金会;

关键词：

EVENTS;

D O I：

10.3847/1538-4357/ac35d1

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We report the result of a search for neutrinos in coincidence with solar flares from the GOES flare database. The search was performed on a 10.8 kton-year exposure of KamLAND collected from 2002 to 2019. This large exposure allows us to explore previously unconstrained parameter space for solar flare neutrinos. We found no statistical excess of neutrinos and established 90% confidence level upper limits of 8.4 x 10(7) cm(-2) (3.0 x 10(9) cm(-2)) on the electron antineutrino (electron neutrino) fluence at 20 MeV normalized to the X12 flare, assuming that the neutrino fluence is proportional to the X-ray intensity.

引用

页数：10

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