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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 |