Atmospheric Neutrino Fluxes
arXiv:astro-ph/0502380 · doi:10.1088/0031-8949/2005/T121/007
Abstract
Starting with an historical review, I summarize the status of calculations of the flux of atmospheric neutrinos and how they compare to measurements.
14 pages, 8 figures, for Proceedings of Nobel Symposium 129 "Neutrino Physics"
References in corpus (6)
- A Measurement of Atmospheric Neutrino Oscillation Parameters by Super-Kamiokande I
- Evidence for an oscillatory signature in atmospheric neutrino oscillation
- A three-dimensional calculation of atmospheric neutrinos
- Measurements of Primary and Atmospheric Cosmic-Ray Spectra with the BESS-TeV Spectrometer
- A New calculation of the atmospheric neutrino flux in a 3-dimensional scheme
- Measurement of the Atmospheric Muon Spectrum from 20 to 3000 GeV
Cited by in corpus (4)
- Multi-year search for a diffuse flux of muon neutrinos with AMANDA-II
- Upper Limits to Fluxes of Neutrinos and Gamma-Rays from Starburst Galaxies
- First Detailed Calculation of Atmospheric Neutrino Foregrounds to the Diffuse Supernova Neutrino Background in Super-Kamiokande
- Study of the homogeneous Bethe-Salpeter equation in the 2+1 Minkowski space