2004/03/11 by B. Bekman, J. Holeczek, J. Kisiel
Physics and Astronomy · #hep-ph
published as Acta Phys.Polon. B35 (2004) 1215-1222 · Postscript file: 7 pages, 2 figures; tar-compressed file: tex source code, eps figures. To appear in Acta. Phys. Pol. B. Talk given at the XXVIII Mazurian Lakes School of Physics, Krzyze, Poland, August 31 - September 7, 2003
arxiv created 2004/03/11 · arxiv updated 2009/12/01
Matter effects on neutrino oscillations in both, a supernova and the Earth, change the observed supernova neutrino spectra. We calculate the expected number of supernova neutrino interactions for ICARUS, SK and SNO detectors as a function of the distance which they traveled in the Earth. Calculations are performed for supernova type II at 10kpc from the Earth, using standard supernova neutrino fluxes described by thermal Fermi--Dirac distributions and the PREM I Earth matter density profile.