Flux of Atmospheric Neutrinos

Details Flux of Atmospheric Neutrinos Flux of Atmospheric Neutrinos

2002-03-29

arxiv.org/abs/hep-ph/0203272v2

Ann.Rev.Nucl.Part.Sci.52:153-199,2002

Physics

High Energy Physics

High Energy Physics - Phenomenology

68 pages, 26 figures. With permission from the Annual Review of Nuclear & Particle Science. Final version of this material is

Scientific paper

10.1146/annurev.nucl.52.050102.0

Atmospheric neutrinos produced by cosmic-ray interactions in the atmosphere are of interest for several reasons. As a beam for studies of neutrino oscillations they cover a range of parameter space hitherto unexplored by accelerator neutrino beams. The atmospheric neutrinos also constitute an important background and calibration beam for neutrino astronomy and for the search for proton decay and other rare processes. Here we review the literature on calculations of atmospheric neutrinos over the full range of energy, but with particular attention to the aspects important for neutrino oscillations. Our goal is to assess how well the properties of atmospheric neutrinos are known at present.

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