A new calculation of atmospheric neutrino flux
We calculate and analyse the atmospheric neutrino flux with a threedimensional Monte Carlo calculation including muon polarization effect. The flux ratio has a plateau ve/vμ = 0.49. This value is not enough to explain the Kamioka data. We present the expected neutrino fluxes at several detector sites.
PACS95.90 Other topics in astronomy and astrophysics
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- T. Gaisser, T. Stanev, S. Bludman andH. Lee:Phys. Rev. Lett,51, 223 (1983); inFourth Workshop on Grand Unification, edited byH. A. Weldon, P. Langacker andP. J. Steinhardt (Birkhauser, Boston, Mass., 1983);T. K. Gaisser andT. Stanev: inICOBAN 1984, Proceedings of the International Colloquium on Baryon Nonconservation,Salt Lake City, edited byD. Cline (University of Wisconsin, Madison, WI, 1984).ADSCrossRefGoogle Scholar
- T. K. Gaisser, R. J. Protheroe andT. Stanev: inProceedings of the XVIII International Cosmic Ray Conference, Bangalore, India, 1983, edited byN. Durgaprasad et al., Vol.5 (Tata Institute of Fundamental Research, Bombay, 1983), p. 174.Google Scholar