The geometry of atmospheric neutrino production

  • Paolo Lipari
  • Published 2000


The zenith angle distributions of atmospheric neutrinos are determined by the possible presence of neutrino oscillations and the combination of three most important contributions: (1) geomagnetic effects on the primary cosmic rays, that suppress the primary flux in the Earth’s magnetic equatorial region, (2) the zenith angle dependence of the neutrino… (More)


11 Figures and Tables