A 3-Dimensional Atmospheric Neutrino Flux Calculation

Details A 3-Dimensional Atmospheric Neutrino Flux Calculation A 3-Dimensional Atmospheric Neutrino Flux Calculation

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....3.1411b&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

A full 3-dimensional code has been developed within the framework of the Bartol atmospheric neutrino flux calculations [1,2], which until now have been made in the one-dimensional approximation. Bending of primaries and secondaries within a realistic geomagnetic field is included. The ultimate goal is to provide a new set of neutrino fluxes for use in interpretation of measurements of atmospheric neutrinos [3,4] and derivation of oscillation parameters. Here we mention some features of the calculational scheme and use it to illustrate the basic features of a three-dimensional calculation.

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