Reducing uncertainty in atmospheric neutrino flux prediction

M. Honda, T. Kajita, K. Kasahara, S. Midorikawa, T. Sanuki, J. Nishimura, A. Okada

研究成果: Paper査読

1 被引用数 (Scopus)

抄録

The atmospheric neutrino is still an important tool in the study of neutrino physics. The uncertainty of the predicted atmospheric neutrino flux is caused by the uncertainties in the physical assumptions and in the calculation scheme. We discuss them quantitatively, and present the works to reduce them. The uncertainty related to the hadronic interaction model was discussed before, therefore, we mainly study other uncertainty sources than the hadronic interaction model here.

本文言語English
ページ1491-1494
ページ数4
出版ステータスPublished - 2007
外部発表はい
イベント30th International Cosmic Ray Conference, ICRC 2007 - Merida, Yucatan, Mexico
継続期間: 2007 7 32007 7 11

Other

Other30th International Cosmic Ray Conference, ICRC 2007
国/地域Mexico
CityMerida, Yucatan
Period07/7/307/7/11

ASJC Scopus subject areas

  • 核物理学および高エネルギー物理学

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