A 3-D Calculation of Atmospheric Neutrino Fluxes

Details A 3-D Calculation of Atmospheric Neutrino Fluxes A 3-D Calculation of Atmospheric Neutrino Fluxes

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....3.1196t&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

We present a fully three-dimensional calculation of atmospheric neutrino fluxes using accurate models of the geomagnetic field, hadronic interactions, tracking and decays. Results are presented for the Super-Kamiokande (SK) and Sudbury Neutrino Observatory (SNO) sites, and we make a comparison with previous one-dimensional calculations. The recently reported geometrical enhancement of low energy, horizontal neutrinos is confirmed, and east-west asymmetries calculated.

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