Reducing uncertainty in atmospheric neutrino flux prediction

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

Research output: Contribution to conferencePaperpeer-review

2 Citations (Scopus)


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.

Original languageEnglish
Number of pages4
Publication statusPublished - 2007
Externally publishedYes
Event30th International Cosmic Ray Conference, ICRC 2007 - Merida, Yucatan, Mexico
Duration: 2007 Jul 32007 Jul 11


Other30th International Cosmic Ray Conference, ICRC 2007
CityMerida, Yucatan

ASJC Scopus subject areas

  • Nuclear and High Energy Physics


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