Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientific paper
2011-02-14
Phys.Rev.D83:123001,2011
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
46 pages, 28 figures
Scientific paper
10.1103/PhysRevD.83.123001
We present the calculation of the atmospheric neutrino fluxes with an interaction model named JAM, which is used in PHITS (Particle and Heavy-Ion Transport code System). The JAM interaction model agrees with the HARP experiment a little better than DPMJET-III. After some modifications, it reproduces the muon flux below 1~GeV/c at balloon altitudes better than the modified-DPMJET-III which we used for the calculation of atmospheric neutrino flux in previous works. Some improvements in the calculation of atmospheric neutrino flux are also reported.
Honda Morihiro
Kajita Takaaki
Kasahara Katsuaki
Midorikawa Shoichi
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