Supernova relic neutrino search at super-Kamiokande

被引：153

作者：

Bays, K. ^{[6
]}

Iida, T. ^{[1
]}

Abe, K. ^{[1
]}

Hayato, Y. ^{[1
,3
]}

Iyogi, K. ^{[1
]}

Kameda, J. ^{[1
]}

Koshio, Y. ^{[1
]}

Marti, L. ^{[1
]}

Miura, M. ^{[1
]}

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

Nakahata, M. ^{[1
,3
]}

Nakayama, S. ^{[1
]}

Obayashi, Y. ^{[1
]}

Sekiya, H. ^{[1
]}

Shiozawa, M. ^{[1
,3
]}

Suzuki, Y. ^{[1
,3
]}

Takeda, A. ^{[1
]}

Takenaga, Y. ^{[1
]}

Ueno, K. ^{[1
]}

Ueshima, K. ^{[1
]}

Yamada, S. ^{[1
]}

Yokozawa, T. ^{[1
]}

Kaji, H. ^{[2
]}

Kajita, T. ^{[2
,3
]}

Kaneyuki, K. ^{[2
,3
]}

McLachlan, T. ^{[2
]}

Okumura, K. ^{[2
]}

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

Martens, K. ^{[3
]}

Vagins, M. ^{[3
,6
]}

Labarga, L. ^{[4
]}

Kearns, E. ^{[3
,5
]}

Litos, M. ^{[5
]}

Raaf, J. L. ^{[5
]}

Stone, J. L. ^{[3
,5
]}

Sulak, L. R. ^{[5
]}

Kropp, W. R. ^{[6
]}

Mine, S. ^{[6
]}

Regis, C. ^{[6
]}

Renshaw, A. ^{[6
]}

Smy, M. B. ^{[3
,6
]}

Sobel, H. W. ^{[3
,6
]}

Ganezer, K. S. ^{[7
]}

Hill, J. ^{[7
]}

Keig, W. E. ^{[7
]}

Cho, S. ^{[7
]}

Jang, J. S. ^{[8
]}

Kim, J. Y. ^{[8
]}

Lim, I. T. ^{[8
]}

Albert, J. ^{[8
]}

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 Tokyo, Todai Inst Adv Study, Inst Phys & Math Universe, Kashiwa, Chiba 2778582, Japan

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

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

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

[7] Calif State Univ, Dept Phys, Carson, CA 90747 USA

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

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

[10] Fukuoka Inst Technol, Jr Coll, Fukuoka 8110214, Japan

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

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

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

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

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

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

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

[18] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA

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

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

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

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

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

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

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

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

[27] Univ Warsaw, Inst Expt Phys, PL-00681 Warsaw, Poland

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

来源：

PHYSICAL REVIEW D | 2012年 / 85卷 / 05期

基金：

中国国家自然科学基金; 新加坡国家研究基金会; 美国能源部; 日本学术振兴会; 美国国家科学基金会;

关键词：

EVOLUTION;

D O I：

10.1103/PhysRevD.85.052007

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A new Super-Kamiokande search for supernova relic neutrinos was conducted using 2853 live days of data. Sensitivity is now greatly improved compared to the 2003 Super-Kamiokande result, which placed a flux limit near many theoretical predictions. This more detailed analysis includes a variety of improvements such as increased efficiency, a lower energy threshold, and an expanded data set. New combined upper limits on supernova relic neutrino flux are between 2.8 and 3.1 (v) over bar (e) cm(-2) s(-1) > 16 MeV total positron energy (17.3 MeV E-v).

引用

页数：15

共 33 条

[1] A search for neutrinos from the solar hep reaction and the diffuse supernova neutrino background with the Sudbury Neutrino Observatory [J].

Aharmim, B. ;

Ahmed, S. N. ;

Anthony, A. E. ;

Beier, E. W. ;

Bellerive, A. ;

Bergevin, M. ;

Biller, S. D. ;

Boulay, M. G. ;

Chan, Y. D. ;

Chen, M. ;

Chen, X. ;

Cleveland, B. T. ;

Cox, G. A. ;

Currat, C. A. ;

Dai, X. ;

Dalnoki-Veress, F. ;

Deng, H. ;

Detwiler, J. ;

DiMarco, M. ;

Doe, P. J. ;

Doucas, G. ;

Drouin, P. -L. ;

Duncan, F. A. ;

Dunford, M. ;

Dunmore, J. A. ;

Earle, E. D. ;

Evans, H. C. ;

Ewan, G. T. ;

Farine, J. ;

Fergani, H. ;

Fleurot, F. ;

Ford, R. J. ;

Formaggio, J. A. ;

Gagnon, N. ;

Goon, J. Tm. ;

Graham, K. ;

Guillian, E. ;

Hahn, R. L. ;

Hallin, A. L. ;

Hallman, E. D. ;

Harvey, P. J. ;

Hazama, R. ;

Heeger, K. M. ;

Heintzelman, W. J. ;

Heise, J. ;

Helmer, R. L. ;

Hemingway, R. J. ;

Henning, R. ;

Hime, A. ;

Howard, C. .

ASTROPHYSICAL JOURNAL, 2006, 653 (02) :1545-1551

[2] Detectability of the supernova relic neutrinos and neutrino oscillation [J].

Ando, S ;

Sato, K ;

Totani, T .

ASTROPARTICLE PHYSICS, 2003, 18 (04) :307-318

[3] Measurement of atmospheric neutrino oscillation parameters by Super-Kamiokande I [J].

Ashie, Y ;

Hosaka, J ;

Ishihara, K ;

Itow, Y ;

Kameda, J ;

Koshio, Y ;

Minamino, A ;

Mitsuda, C ;

Miura, M ;

Moriyama, S ;

Nakahata, M ;

Namba, T ;

Nambu, R ;

Obayashi, Y ;

Shiozawa, M ;

Suzuki, Y ;

Takeuchi, Y ;

Taki, K ;

Yamada, S ;

Ishitsuka, M ;

Kajita, T ;

Kaneyuki, K ;

Nakayama, S ;

Okada, A ;

Okumura, K ;

Saji, C ;

Takenaga, Y ;

Clark, ST ;

Desai, S ;

Kearns, E ;

Likhoded, S ;

Stone, JL ;

Sulak, LR ;

Wang, W ;

Goldhaber, M ;

Casper, D ;

Cravens, JP ;

Gajewski, W ;

Kropp, WR ;

Liu, DW ;

Mine, S ;

Smy, MB ;

Sobel, HW ;

Sterner, CW ;

Vagins, MR ;

Ganezer, KS ;

Hill, J ;

Keig, WE ;

Jang, JS ;

Kim, JY .

PHYSICAL REVIEW D, 2005, 71 (11)

[4] Antineutrino spectroscopy with large water Cerenkov detectors [J].

Beacom, JF ;

Vagins, MR .

PHYSICAL REVIEW LETTERS, 2004, 93 (17) :171101-1

[5] The Diffuse Supernova Neutrino Background [J].

Beacom, John F. .

ANNUAL REVIEW OF NUCLEAR AND PARTICLE SCIENCE, VOL 60, 2010, 60 :439-462

[6] SUPERNOVAE, NEUTRINO REST MASS, AND THE MIDDLE-ENERGY NEUTRINO BACKGROUND IN THE UNIVERSE [J].

BISNOVATYIKOGAN, GS ;

SEIDOV, ZF .

ANNALS OF THE NEW YORK ACADEMY OF SCIENCES, 1984, 422 (MAR) :319-327

[7]

Blaufuss E, 2001, NUCL INSTRUM METH A, V458, P638, DOI 10.1016/S0168-9002(00)00900-1

[8]

Cappellaro E, 1999, ASTRON ASTROPHYS, V351, P459

[9] Solar neutrino measurements in Super-Kamiokande-II [J].

Cravens, J. P. ;

Abe, K. ;

Iida, T. ;

Ishihara, K. ;

Kameda, J. ;

Koshio, Y. ;

Minamino, A. ;

Mitsuda, C. ;

Miura, M. ;

Moriyama, S. ;

Nakahata, M. ;

Nakayama, S. ;

Obayashi, Y. ;

Ogawa, H. ;

Sekiya, H. ;

Shiozawa, M. ;

Suzuki, Y. ;

Takeda, A. ;

Takeuchi, Y. ;

Ueshima, K. ;

Watanabe, H. ;

Yamada, S. ;

Higuchi, I. ;

Ishihara, C. ;

Ishitsuka, M. ;

Kajita, T. ;

Kaneyuki, K. ;

Mitsuka, G. ;

Nishino, H. ;

Okumura, K. ;

Saji, C. ;

Takenaga, Y. ;

Clark, S. ;

Desai, S. ;

Dufour, F. ;

Kearns, E. ;

Likhoded, S. ;

Litos, M. ;

Raaf, J. L. ;

Stone, J. L. ;

Sulak, L. R. ;

Wang, W. ;

Goldhaber, M. ;

Casper, D. ;

Dunmore, J. ;

Kropp, W. R. ;

Liu, D. W. ;

Mine, S. ;

Regis, C. ;

Smy, M. B. .

PHYSICAL REVIEW D, 2008, 78 (03)

[10] The Super-Kamiokande detector [J].

Fukuda, S ;

Fukuda, Y ;

Hayakawa, T ;

Ichihara, E ;

Ishitsuka, M ;

Itow, Y ;

Kajita, T ;

Kameda, J ;

Kaneyuki, K ;

Kasuga, S ;

Kobayashi, K ;

Kobayashi, Y ;

Koshio, Y ;

Miura, M ;

Moriyama, S ;

Nakahata, M ;

Nakayama, S ;

Namba, T ;

Obayashi, Y ;

Okada, A ;

Oketa, M ;

Okumura, K ;

Oyabu, T ;

Sakurai, N ;

Shiozawa, M ;

Suzuki, Y ;

Takeuchi, Y ;

Toshito, T ;

Totsuka, Y ;

Yamada, S ;

Desai, S ;

Earl, M ;

Hong, JT ;

Kearns, E ;

Masuzawa, M ;

Messier, MD ;

Stone, JL ;

Sulak, LR ;

Walter, CW ;

Wang, W ;

Scholberg, K ;

Barszczak, T ;

Casper, D ;

Liu, DW ;

Gajewski, W ;

Halverson, PG ;

Hsu, J ;

Kropp, WR ;

Mine, S ;

Price, LR .

NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 2003, 501 (2-3) :418-462

← 1 2 3 4 →