ICECUBE OBSERVATORY: NEUTRINOS AND THE ORIGIN OF COSMIC RAYS

dc.contributor.author	Desiati, Paolo
dc.date.accessioned	2021-12-01T13:27:12Z
dc.date.available	2021-12-01T13:27:12Z
dc.date.issued	2013
dc.identifier.citation	Acta Polytechnica. 2013, vol. 53, no. A, p. 770-775.
dc.identifier.issn	1210-2709 (print)
dc.identifier.issn	1805-2363 (online)
dc.identifier.uri	http://hdl.handle.net/10467/98685
dc.description.abstract	The completed IceCube Observatory, the first km3 neutrino telescope, is already providing the most stringent limits on the flux of high energy cosmic neutrinos from point-like and diffuse galactic and extra-galactic sources. The non-detection of extra-terrestrial neutrinos has important consequences on the origin of the cosmic rays. Here the current status of astrophysical neutrino searches, and of the observation of a persistent cosmic ray anisotropy above 100TeV, are reviewed.	en
dc.format.mimetype	application/pdf
dc.language.iso	eng
dc.publisher	České vysoké učení technické v Praze	cs
dc.publisher	Czech Technical University in Prague	en
dc.relation.ispartofseries	Acta Polytechnica
dc.relation.uri	https://ojs.cvut.cz/ojs/index.php/ap/article/view/1983
dc.rights	Creative Commons Attribution 4.0 International License	en
dc.rights.uri	http://creativecommons.org/licenses/by/4.0/
dc.title	ICECUBE OBSERVATORY: NEUTRINOS AND THE ORIGIN OF COSMIC RAYS
dc.type	article	en
dc.date.updated	2021-12-01T13:27:12Z
dc.identifier.doi	10.14311/AP.2013.53.0770
dc.rights.access	openAccess
dc.type.status	Peer-reviewed
dc.type.version	publishedVersion

Except where otherwise noted, this item's license is described as Creative Commons Attribution 4.0 International License