Calculation of the atmospheric neutrino flux improved with recent cosmic ray observations

Details Calculation of the atmospheric neutrino flux improved with recent cosmic ray observations Calculation of the atmospheric neutrino flux improved with recent cosmic ray observations

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....3.1162h&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

1

Scientific paper

The primary cosmic ray spectrum below 100 GeV has been measured very accurately by the recent experiment, such as BESS and AMS. Also the measurements of secondary cosmic rays such as muons and gamma rays are extensively carried out in order to improve the prediction of atmospheric neutrino flux. Using the results of accurately measured cosmic ray fluxes, we revise the hadronic interaction model and calculate the atmospheric neutrino flux.

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