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Uncertainty of the atmospheric neutrino fluxes

โœ Scribed by M. Honda


Publisher
Elsevier Science
Year
1999
Tongue
English
Weight
434 KB
Volume
77
Category
Article
ISSN
0920-5632

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โœฆ Synopsis


The uncertainty in the calculation of atmospheric neutrino fluxes is studied. The absolute value of atmospheric neutrino fluxes is sensitive to variation of the primary cosmic ray flux model asld/or the interaction model. However, the ratios between different kind of neutrinos stay almost unchanged with these variations. It is unlikely that the anomalous ratio (u~,/u~)ob~/(v~,/t~,)MC reported by Kamiokande and Super Kamiokande is caused by the uncertainty of predicted atmospheric neutrino fluxes.


๐Ÿ“œ SIMILAR VOLUMES


Atmospheric Neutrino Fluxes
โœ Giles Barr ๐Ÿ“‚ Article ๐Ÿ“… 2005 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 270 KB
Atmospheric neutrino fluxes
โœ Thomas K. Gaisser ๐Ÿ“‚ Article ๐Ÿ“… 2003 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 766 KB

This talk is a status report on calculations of the flux of atmospheric neutrinos from the sub-GeV range to Ev N PeV. In the lower energy range (E, < 1 TeV) the primary interest is in using the atmospheric neutrino beam to study neutrino oscillations. In the TeV range and above, atmospheric neutrino