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Limits on the diffuse flux of ultra-high energy neutrinos using the Pierre Auger Observatory

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Limits on the diffuse flux of ultra-high energy neutrinos using the Pierre Auger Observatory

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dc.contributor.author The Pierre Auger Collaboration
dc.contributor.author Pastor Carpi, Sergio
dc.date.accessioned 2014-09-03T09:45:57Z
dc.date.available 2014-09-03T09:45:57Z
dc.date.issued 2012
dc.identifier.citation The Pierre Auger Collaboration Pastor Carpi, Sergio 2012 Limits on the diffuse flux of ultra-high energy neutrinos using the Pierre Auger Observatory Nuclear Instruments & Methods in Physics Research Section A-Accelerators Spectrometers Detectors and Associated Equipment 662 S113 S117
dc.identifier.uri http://hdl.handle.net/10550/37487
dc.description.abstract The surface detector array of the Pierre Auger Observatory is sensitive to ultra-high energy neutrinos in the cosmic radiation. These particles can interact close to ground, both through charged and neutral currents in the atmosphere (down-going) and, for tau neutrinos, through the Earth-skimming mechanism (up-going) where a tau lepton is produced in the Earth's crust that can emerge and decay in the atmosphere. Both types of neutrino-induced events produce an inclined shower that can be identified by the presence of a broad time structure of signals in the water-Cherenkov detectors. Using data collected from the surface detector array of the Pierre Auger Observatory, we present the corresponding limits on the diffuse flux of ultra-high energy neutrinos.
dc.language.iso eng
dc.relation.ispartof Nuclear Instruments & Methods in Physics Research Section A-Accelerators Spectrometers Detectors and Associated Equipment, 2012, vol. 662, p. S113-S117
dc.subject Física
dc.title Limits on the diffuse flux of ultra-high energy neutrinos using the Pierre Auger Observatory
dc.type journal article es_ES
dc.date.updated 2014-09-03T09:45:57Z
dc.identifier.doi 10.1016/j.nima.2010.11.014
dc.identifier.idgrec 078461
dc.rights.accessRights open access es_ES

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