Search forν¯efrom the Sun at Super-Kamiokande-I
Copyright policy ) T. Ishizuka; Hyosun Kim; T. J. Haines; T. J. Haines; K. Nakamura; J. L. Stone; S. C. Boyd; +121 Authors
T. Ishizuka; Hyosun Kim; T. J. Haines; T. J. Haines; K. Nakamura; J. L. Stone; S. C. Boyd; A. K. Ichikawa; J. Kameda; Shantanu Desai; H. Okazawa; R. W. Ellsworth; S. Mine; Masato Shiozawa; C. W. Walter; A. Suzuki; A. T. Suzuki; Y. Fukuda; Y. Hayato; K. Nitta; T. Toshito; K. Nishikawa; W. R. Kropp; Ken-ichiro Kobayashi; Tomoyuki Maruyama; I. Kato; Masayuki Nakahata; J. Shirai; R. J. Wilkes; G. W. Sullivan; R. Svoboda; S. B. Kim; R. Nishimura; M. Kohama; M. Ishitsuka; M. R. Vagins; M. Koike; M. Etoh; Alec Habig; T. Iwashita; Hirokazu Ishino; D. W. Liu; Mikio Morii; Kazumasa Miyano; John G. Learned; B. Viren; B. Viren; Y. Takeuchi; M. Ackermann; M. Goldhaber; Y. Nagashima; T. Inagaki; K. Martens; K. Martens; Tsuyoshi Nakaya; Y. Gando; Yasunari Suzuki; S. Dazeley; G. Guillian; M. Koshiba; Takehisa Hasegawa; K. Ishihara; Y. Ichikawa; H. G. Berns; L. R. Sulak; H. W. Sobel; Toshio Namba; Y. Watanabe; J. A. Goodman; E. Sharkey; T. Ishii; D. Kielczewska; D. Kielczewska; S. Matsuno; K. Nishijima; Takaaki Kajita; David William Casper; M. L. Chen; Makoto Sakuda; C. Yanagisawa; A. L. Stachyra; W. Gajewski; T. Kobayashi; S. Fukuda; C. Mitsuda; Y. Kajiyama; M. D. Messier; M. D. Messier; C. Saji; E. Kearns; D. Turcan; J. Hill; M. Earl; C. McGrew; Yusuke Koshio; Magdalena Malek; C. K. Jung; C. Mauger; M. Takita; H. Takeuchi; K. Kaneyuki; D. Takemori; Nobuyuki Sakurai; Y. Hatakeyama; Kate Scholberg; Michitoshi Yoshida; Shigeki Tasaka; E. Blaufuss; T. Ooyabu; Yoshitaka Itow; T. Shibata; S. Yamada; K. S. Ganezer; M. Miura; Y. Obayashi; Yuichi Oyama; J. Yoo; Kunio Inoue; S. Hatakeyama; Y. Totsuka; T. Barszczak; S. Nakayama; A. Gago; M. B. Smy; A. Kibayashi; A. Okada; W. E. Keig; S. Moriyama;
Search forν¯efrom the Sun at Super-Kamiokande-I
We present the results of a search for low energy nu(e) from the Sun using 1496 days of data from Super-Kamiokande-I. We observe no significant excess of events and set an upper limit for the conversion probability to nu(e) of the 8B solar neutrino. This conversion limit is 0.8% (90% C.L.) of the standard solar model's neutrino flux for total energy=8-20 MeV. We also set a flux limit for monochromatic nu(e) for E(nu(e))=10-17 MeV.
- Seoul National University Korea (Republic of)
- Kyoto University Japan
- University of Mary United States
- Tohoku University Japan
- Seoul National University Korea (Republic of)
citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).54 popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.Top 10% influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).Top 10% impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.Top 10%
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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
Citations provided by BIP!popularityPopularity provided by BIP!
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
Popularity provided by BIP! 54
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