Expected Angular Distribution of Atmospheric Muons at Super-Kamiokande Detector

Details Expected Angular Distribution of Atmospheric Muons at Super-Kamiokande Detector Expected Angular Distribution of Atmospheric Muons at Super-Kamiokande Detector

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....3.1467b&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

The angular distribution of atmospheric muons at the site of superKamiokande (Sup erK) detector was calculated using a set of three-dimensional Monte-Carlo codes for muon propagation. These codes include recent treatment of multiple Coulomb scattering of muons and new consideration of cross section of inelastic muon interaction in matter. Results of simulation are compared with superK data near the horizontal direction.

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