Solar 8B and hep neutrino measurements from 1258 days of Super-Kamiokande data

被引:996
作者
Fukuda, S
Fukuda, Y
Ishitsuka, M
Itow, Y
Kajita, T
Kameda, J
Kaneyuki, K
Kobayashi, K
Koshio, Y
Miura, M
Moriyama, S
Nakahata, M
Nakayama, S
Okada, A
Sakurai, N
Shiozawa, M
Suzuki, Y
Takeuchi, H
Takeuchi, Y
Toshito, T
Totsuka, Y
Yamada, S
Desai, S
Earl, M
Kearns, E
Messier, MD
Scholberg, K [1 ]
Stone, JL
Sulak, LR
Walter, CW
Goldhaber, M
Barszczak, T
Casper, D
Gajewski, W
Kropp, WR
Mine, S
Liu, DW
Price, LR
Smy, MB
Sobel, HW
Vagins, MR
Ganezer, KS
Keig, WE
Ellsworth, RW
Tasaka, S
Kibayashi, A
Learned, JG
Matsuno, S
Takemori, D
Hayato, Y
机构
[1] Univ Tokyo, Inst Cosm Ray Res, Kashiwa, Chiba 2778582, Japan
[2] Boston Univ, Dept Phys, Boston, MA 02215 USA
[3] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA
[4] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA
[5] Calif State Univ Dominguez Hills, Dept Phys, Carson, CA 90747 USA
[6] George Mason Univ, Dept Phys, Fairfax, VA 22030 USA
[7] Gifu Univ, Dept Phys, Gifu 5011193, Japan
[8] Univ Hawaii, Dept Phys & Astron, Honolulu, HI 96822 USA
[9] High Energy Accelerator Res Org, Inst Particle & Nucl Studies, Tsukuba, Ibaraki 3050801, Japan
[10] Kobe Univ, Dept Phys, Kobe, Hyogo 6578501, Japan
[11] Kyoto Univ, Dept Phys, Kyoto 6068502, Japan
[12] Los Alamos Natl Lab, Div Phys, Los Alamos, NM 87544 USA
[13] Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA
[14] Univ Maryland, Dept Phys, College Pk, MD 20742 USA
[15] Univ Minnesota, Dept Phys, Duluth, MN 55812 USA
[16] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA
[17] Niigata Univ, Dept Phys, Niigata 9502181, Japan
[18] Osaka Univ, Dept Phys, Toyonaka, Osaka 5600043, Japan
[19] Seoul Natl Univ, Dept Phys, Seoul 151742, South Korea
[20] Shizuoka Seika Coll, Shizuoka 4258611, Japan
[21] Shizuoka Univ, Dept Syst Engn, Hamamatsu, Shizuoka 4328561, Japan
[22] Tohoku Univ, Res Ctr Neutrino Sci, Sendai, Miyagi 9808578, Japan
[23] Univ Tokyo, Tokyo 1130033, Japan
[24] Tokai Univ, Dept Phys, Hiratsuka, Kanagawa 2591292, Japan
[25] Tokyo Inst Technol, Dept Phys, Tokyo 1528551, Japan
[26] Univ Warsaw, Inst Expt Phys, PL-00681 Warsaw, Poland
[27] Univ Washington, Dept Phys, Seattle, WA 98195 USA
关键词
D O I
10.1103/PhysRevLett.86.5651
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Solar neutrino measurements from 1258 days of data from the Super-Kamiokande detector are presented. The measurements are based on recoil electrons in the energy range 5.0-20.0 MeV. The measured solar neutrino flux is 2.32 +/- 0.03(stat)(+0.08)(-0.07) (syst) x 10(6) cm(-2) s(-1) which is 45.1 +/- 0.5 (stat)(+1.6)(-1.4)(syst)% of that predicted by the BP2000 SSM. The day vs nieht flux asymmetry (Phi (n) - Phi (d)) / Phi (average) is 0.033 +/- 0.022(stat)(+0.013)(-0.012)(syst). The recoil electron energy spectrum is consistent with no spectral distortion. For the hep neutrino flux, we set a 90% C.L. upper limit of 40 x 10(3) cm(-2) s(-1) which is 4.3 times the BP2000 SSM prediction.
引用
收藏
页码:5651 / 5655
页数:5
相关论文
共 23 条
[1]   Measurement of the solar neutrino capture rate with gallium metal [J].
Abdurashitov, JN ;
Gavrin, VN ;
Girin, SV ;
Gorbachev, VV ;
Ibragimova, TV ;
Kalikhov, AV ;
Khairnasov, NG ;
Knodel, TV ;
Mirnov, IN ;
Shikhin, AA ;
Veretenkin, EP ;
Vermul, VM ;
Yants, VE ;
Zatsepin, GT ;
Bowles, TJ ;
Teasdale, WA ;
Wark, DL ;
Cherry, ML ;
Nico, JS ;
Cleveland, BT ;
Davis, R ;
Lande, K ;
Wildenhain, PS ;
Elliott, SR ;
Wilkerson, JF .
PHYSICAL REVIEW C, 1999, 60 (05) :32
[2]   GALLEX RESULTS FROM THE 1ST 30 SOLAR-NEUTRINO RUNS [J].
ANSELMANN, P ;
HAMPEL, W ;
HEUSSER, G ;
KIKO, J ;
KIRSTEN, T ;
LAUBENSTEIN, M ;
PERNICKA, E ;
PEZZONI, S ;
RONN, U ;
SANN, M ;
SCHLOSSER, C ;
WINK, R ;
WOJCIK, M ;
VONAMMON, R ;
EBERT, KH ;
FRITSCH, T ;
HELLRIEGEL, K ;
HENRICH, E ;
STIEGLITZ, L ;
WEIRICH, F ;
BALATA, M ;
FERRARI, N ;
LALLA, H ;
BELLOTTI, E ;
CATTADORI, C ;
CREMONESI, O ;
FIORINI, E ;
ZANOTTI, L ;
ALTMANN, M ;
VONFEILITZSCH, F ;
MOSSBAUER, R ;
SCHANDA, U ;
BERTHOMIEU, G ;
SCHATZMAN, E ;
CARMI, I ;
DOSTROVSKY, I ;
BACCI, C ;
BELLI, P ;
BERNABEI, R ;
DANGELO, S ;
PAOLUZI, L ;
BEVILACQUA, A ;
CHARBIT, S ;
CRIBIER, M ;
GOSSET, L ;
RICH, J ;
SPIRO, M ;
STOLARCZYK, T ;
TAO, C ;
VIGNAUD, D .
PHYSICS LETTERS B, 1994, 327 (3-4) :377-385
[3]   Standard neutrino spectrum from B-8 decay [J].
Bahcall, JN ;
Lisi, E ;
Alburger, DE ;
DeBraeckeleer, L ;
Freedman, SJ ;
Napolitano, J .
PHYSICAL REVIEW C, 1996, 54 (01) :411-422
[4]   How uncertain are solar neutrino predictions? [J].
Bahcall, JN ;
Basu, S ;
Pinsonneault, MH .
PHYSICS LETTERS B, 1998, 433 (1-2) :1-8
[5]  
Blaufuss E, 2001, NUCL INSTRUM METH A, V458, P638, DOI 10.1016/S0168-9002(00)00900-1
[6]   MATTER EFFECTS FOR SOLAR NEUTRINO OSCILLATIONS [J].
BOUCHEZ, J ;
CRIBIER, M ;
HAMPEL, W ;
RICH, J ;
SPIRO, M ;
VIGNAUD, D .
ZEITSCHRIFT FUR PHYSIK C-PARTICLES AND FIELDS, 1986, 32 (04) :499-511
[7]   TERRESTRIALLY ENHANCED NEUTRINO OSCILLATIONS [J].
CARLSON, ED .
PHYSICAL REVIEW D, 1986, 34 (05) :1454-1459
[8]  
*CERN PROGR LIB, 1994, GEANT DET DESCR SIM
[9]   Measurement of the solar electron neutrino flux with the Homestake chlorine detector [J].
Cleveland, BT ;
Daily, T ;
Davis, R ;
Distel, JR ;
Lande, K ;
Lee, CK ;
Wildenhain, PS ;
Ullman, J .
ASTROPHYSICAL JOURNAL, 1998, 496 (01) :505-526
[10]   RADIATIVE DECAYS OF THE 16.6 AND 16.9 MEV STATES IN BE-8 AND TESTS OF THE CONSERVATION OF THE VECTOR CURRENT IN THE A=8 MULTIPLET [J].
DEBRAECKELEER, L ;
ADELBERGER, EG ;
GUNDLACH, JH ;
KAPLAN, M ;
MARKOFF, D ;
NATHAN, AM ;
SCHIEFF, W ;
SNOVER, KA ;
STORM, DW ;
SWARTZ, KB ;
WRIGHT, D ;
BROWN, BA .
PHYSICAL REVIEW C, 1995, 51 (05) :2778-2788