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16N as a calibration source for Super-Kamiokande

  • E. Blaufuss
  • , G. Guillian
  • , Y. Fukuda
  • , S. Fukuda
  • , M. Ishitsuka
  • , Y. Itow
  • , T. Kajita
  • , J. Kameda
  • , K. Kaneyuki
  • , K. Kobayashi
  • , Y. Kobayashi
  • , Y. Koshio
  • , M. Miura
  • , S. Moriyama
  • , M. Nakahata
  • , S. Nakayama
  • , Y. Obayashi
  • , A. Okada
  • , K. Okumura
  • , N. Sakurai
  • M. Shiozawa, Y. Suzuki, H. Takeuchi, Y. Takeuchi, T. Toshito, Y. Totsuka, S. Yamada, M. Earl, A. Habig, E. Kearns, M. D. Messier, K. Scholberg, J. L. Stone, L. R. Sulak, C. W. Walter, M. Goldhaber, T. Barszczak, D. Casper, W. Gajewski, W. R. Kropp, S. Mine, L. R. Price, M. Smy, H. W. Sobel, M. R. Vagins, K. S. Ganezer, W. E. Keig, R. W. Ellsworth, S. Tasaka, A. Kibayashi, J. G. Learned, S. Matsuno, D. Takemori, Y. Hayato, T. Ishii, T. Kobayashi, K. Nakamura, Y. Oyama, A. Sakai, M. Sakuda, O. Sasaki, S. Echigo, M. Kohama, A. T. Suzuki, T. Inagaki, K. Nishikawa, T. J. Haines, B. K. Kim, R. Sanford, R. Svoboda, M. L. Chen, J. A. Goodman, G. W. Sullivan, J. Hill, C. K. Jung, K. Martens, M. Malek, C. Mauger, C. McGrew, E. Sharkey, B. Viren, C. Yanagisawa, M. Kirisawa, S. Inaba, C. Mitsuda, K. Miyano, H. Okazawa, C. Saji, M. Takahashi, M. Takahata, Y. Nagashima, K. Nitta, M. Takita, M. Yoshida, S. B. Kim, M. Etoh, Y. Gando, T. Hasegawa, K. Inoue
  • Louisiana State University
  • University of Maryland, College Park
  • The University of Tokyo
  • Boston University
  • Brookhaven National Laboratory
  • University of California at Irvine
  • California State University Dominguez Hills
  • George Mason University
  • Gifu University
  • University of Hawai'i at Mānoa
  • High Energy Accelerator Research Organization, Institute of Particle and Nuclear Physics
  • Kobe University
  • Kyoto University
  • Los Alamos National Laboratory
  • Stony Brook University
  • Niigata University
  • The University of Osaka
  • Seoul National University
  • Tohoku University

Research output: Contribution to journalArticlepeer-review

31 Scopus citations

Abstract

The decay of 16N is used to cross check the absolute energy scale calibration for solar neutrinos established by the electron linear accelerator (LINAC). A deuterium-tritium neutron generator was employed to create 16N via the (n,p) reaction on 16O in the water of the detector. This technique is isotropic and has different systematic uncertainties than the LINAC. The results from this high-statistics data sample agree with the absolute energy scale of the LINAC to better than 1%. A natural source of 16N from the capture of μ- on 16O, which is collected as a background to the solar neutrino analysis, is also discussed.

Original languageEnglish
Pages (from-to)638-649
Number of pages12
JournalNuclear Inst. and Methods in Physics Research, A
Volume458
Issue number3
DOIs
StatePublished - Feb 11 2001

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