Search for Neutrinos from Annihilation of Captured Low-Mass Dark Matter Particles in the Sun by Super-Kamiokande

被引：187

作者：

Choi, K. ^{[19
]}

Abe, K. ^{[1
,30
]}

Haga, Y. ^{[1
]}

Hayato, Y. ^{[1
,30
]}

Iyogi, K. ^{[1
]}

Kameda, J. ^{[1
,2
,30
]}

Kishimoto, Y. ^{[1
,30
]}

Miura, M. ^{[1
]}

Moriyama, S. ^{[1
,30
]}

Nakahata, M. ^{[1
]}

Nakano, Y. ^{[1
]}

Nakayama, S. ^{[1
,30
]}

Sekiya, H. ^{[1
,30
]}

Shiozawa, M. ^{[1
]}

Suzuki, Y. ^{[1
,30
]}

Takeda, A. ^{[1
,30
]}

Tomura, T. ^{[1
,30
]}

Wendell, R. A. ^{[1
,30
]}

Irvine, T. ^{[2
]}

Kajita, T. ^{[2
,30
]}

Kametani, I. ^{[2
]}

Kaneyuki, K. ^{[2
,30
]}

Lee, K. P. ^{[2
]}

Nishimura, Y. ^{[2
]}

Okumura, K. ^{[2
,30
]}

McLachlan, T. ^{[2
]}

Labarga, L. ^{[3
]}

Kearns, E. ^{[4
]}

Raaf, J. L. ^{[4
]}

Stone, J. L. ^{[4
,30
]}

Sulak, L. R. ^{[4
]}

Berkman, S. ^{[5
]}

Tanaka, H. A. ^{[5
]}

Tobayama, S. ^{[5
]}

Goldhaber, M. ^{[6
]}

Carminati, G. ^{[7
]}

Kropp, W. R. ^{[7
]}

Mine, S. ^{[7
]}

Renshaw, A. ^{[7
]}

Smy, M. B. ^{[7
,30
]}

Sobel, H. W. ^{[7
,30
]}

Ganezer, K. S. ^{[8
]}

Hill, J. ^{[8
]}

Hong, N. ^{[9
]}

Kim, J. Y. ^{[9
]}

Lim, I. T. ^{[9
]}

Akiri, T. ^{[10
]}

Himmel, A. ^{[10
]}

Scholberg, K. ^{[10
,30
]}

Walter, C. W. ^{[10
,30
]}

机构：

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

[2] Univ Tokyo, Inst Cosm Ray Res, Res Ctr Cosm Neutrinos, Kashiwa, Chiba 2778582, Japan

[3] Univ Autonoma Madrid, Dept Theoret Phys, E-28049 Madrid, Spain

[4] Boston Univ, Dept Phys, Boston, MA 02215 USA

[5] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z4, Canada

[6] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA

[7] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA

[8] Calif State Univ Dominguez Hills, Dept Phys, Carson, CA 90747 USA

[9] Chonnam Natl Univ, Dept Phys, Kwangju 500757, South Korea

[10] Duke Univ, Dept Phys, Durham, NC 27708 USA

[11] Fukuoka Inst Technol, Jr Coll, Fukuoka 8110295, Japan

[12] Gifu Univ, Dept Phys, Gifu 5011193, Japan

[13] Gwangju Inst Sci & Technol, GIST Coll, Gwangju 500712, South Korea

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

[15] High Energy Accelerator Res Org KEK, Tsukuba, Ibaraki 3050801, Japan

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

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

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

[19] Nagoya Univ, Solar Terr Environm Lab, Nagoya, Aichi 4648602, Japan

[20] Natl Ctr Nucl Res, PL-00681 Warsaw, Poland

[21] SUNY Stony Brook, Dept Phys & Astron, New York, NY 11794 USA

[22] Okayama Univ, Dept Phys, Okayama 7008530, Japan

[23] Osaka Univ, Dept Phys, Toyonaka, Osaka 5600043, Japan

[24] Univ Regina, Dept Phys, Regina, SK S4S 0A2, Canada

[25] Seoul Natl Univ, Dept Phys, Seoul 151742, South Korea

[26] Shizuoka Univ Welf, Dept Informat Social Welf, Yaizu, Shizuoka 4258611, Japan

[27] Sungkyunkwan Univ, Dept Phys, Suwon 440746, South Korea

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

[29] Univ Tokyo, Bunkyo Ku, Tokyo 1130033, Japan

[30] Univ Tokyo, Todai Inst Adv Study, Kavli Inst Phys & Math Universe WPI, Kashiwa, Chiba 2778582, Japan

[31] Univ Toronto, Dept Phys, Toronto, ON M5S 1A7, Canada

[32] TRIUMF, Vancouver, BC V6T 2A3, Canada

[33] Tsinghua Univ, Dept Engn Phys, Beijing 100084, Peoples R China

[34] Univ Washington, Dept Phys, Seattle, WA 98195 USA

来源：

PHYSICAL REVIEW LETTERS | 2015年 / 114卷 / 14期

基金：

美国国家科学基金会;

关键词：

CONSTRAINTS; CANDIDATES; LIMITS;

D O I：

10.1103/PhysRevLett.114.141301

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Super-Kamiokande (SK) can search for weakly interacting massive particles (WIMPs) by detecting neutrinos produced from WIMP annihilations occurring inside the Sun. In this analysis, we include neutrino events with interaction vertices in the detector in addition to upward-going muons produced in the surrounding rock. Compared to the previous result, which used the upward-going muons only, the signal acceptances for light (few-GeV/c(2)-200-GeV/c(2)) WIMPs are significantly increased. We fit 3903 days of SK data to search for the contribution of neutrinos from WIMP annihilation in the Sun. We found no significant excess over expected atmospheric-neutrino background and the result is interpreted in terms of upper limits on WIMP-nucleon elastic scattering cross sections under different assumptions about the annihilation channel. We set the current best limits on the spin-dependent WIMP-proton cross section for WIMP masses below 200 GeV/c(2) (at 10 GeV/c(2), 1.49 x 10(-39) cm(2) for chi chi -> (b) over barb and 1.31 x 10(-40) cm(2) for chi chi -> tau(+)tau(-) annihilation channels), also ruling out some fraction of WIMP candidates with spin-independent coupling in the few-GeV/c(2) mass range.

引用

页数：6

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