Anisotropy of the primary cosmic-ray flux in Super-Kamiokande

Simple item page
dc.creatorOyama, Yuichi
dc.date2006-05-01
dc.date2006-05-08
dc.date.accessioned2026-07-07T07:08:19Z
dc.date.available2026-07-07T07:08:19Z
dc.descriptionA first-ever 2-dimensional celestial map of primary cosmic-ray flux was obtained from 2.10x10^8 cosmic-ray muons accumulated in 1662.0 days of Super-Kamiokande. The celestial map indicates an (0.104 \pm 0.020)% excess region in the constellation of Taurus and a -(0.094 \pm 0.014)% deficit region toward Virgo. Interpretations of this anisotropy are discussed.
dc.description14 pages, 6 figures. Talk at "Les Rencontres de Physique de la Vallee d'Aosta (La Thuile 2006)", La Thuile, Aosta Valley, Italy, March 5-11, 2006
dc.identifierhttps://arxiv.org/abs/astro-ph/0605020
dc.identifierhttp://arxiv.org/abs/astro-ph/0605020
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/110664
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Experiment
dc.titleAnisotropy of the primary cosmic-ray flux in Super-Kamiokande
dc.typetext

Files

Collections

arXiv