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Neutrino searches at the Pierre Auger Observatory

Repositori DSpace/Manakin

dc.contributor.author	Pastor Carpi, Sergio
dc.date.accessioned	2013-11-25T11:53:12Z
dc.date.available	2013-11-25T11:53:12Z
dc.date.issued	2013
dc.identifier.citation	Pastor Carpi, Sergio 2013 Neutrino searches at the Pierre Auger Observatory Nuclear Physics B-Proceedings Supplements 235-236 358 363
dc.identifier.uri	http://hdl.handle.net/10550/31406
dc.description.abstract	The surface detector array of the Pierre Auger Observatory is sensitive to ultra-high energy neutrinos in the cosmic radiation. Neutrinos can interact in the atmosphere close to ground (down-going) and, for tau neutrinos, through the Earth-skimming mechanism (up-going) where a tau lepton is produced in the Earth crust that can emerge and decay in the atmosphere. Both types of neutrino-induced events produce an inclined particle air shower that can be identified by the presence of a broad time structure of signals in the water-Cherenkov detectors. We discuss the neutrino identification criteria used and present the corresponding limits on the diffuse and point-like source fluxes.
dc.relation.ispartof	Nuclear Physics B-Proceedings Supplements, 2013, vol. 235-236, p. 358-363
dc.subject	Partícules (Física nuclear)
dc.title	Neutrino searches at the Pierre Auger Observatory
dc.type	journal article	es_ES
dc.date.updated	2013-11-25T11:53:12Z
dc.identifier.doi	10.1016/j.nuclphysbps.2013.04.033
dc.identifier.idgrec	091171
dc.rights.accessRights	open access	es_ES
dc.identifier.url	10.1016/j.nuclphysbps.2013.04.033