Reducing uncertainty in atmospheric neutrino flux prediction

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

Research output: Contribution to conferencePaperpeer-review

1 Citation (Scopus)

Abstract

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
Pages1491-1494
Number of pages4
Publication statusPublished - 2007 Jan 1
Externally publishedYes
Event30th International Cosmic Ray Conference, ICRC 2007 - Merida, Yucatan, Mexico
Duration: 2007 Jul 32007 Jul 11

Other

Other30th International Cosmic Ray Conference, ICRC 2007
CountryMexico
CityMerida, Yucatan
Period07/7/307/7/11

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

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