Neutrino searches at the Pierre Auger Observatory
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Neutrino searches at the Pierre Auger Observatory

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Neutrino searches at the Pierre Auger Observatory

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Pastor Carpi, Sergio
Aquest document és un/a article, creat/da en: 2013

Este documento está disponible también en : http://dx.doi.org/10.1016/j.nuclphysbps.2013.04.033
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.

    Pastor Carpi, Sergio 2013 Neutrino searches at the Pierre Auger Observatory Nuclear Physics B-Proceedings Supplements 235-236 358 363
http://dx.doi.org/10.1016/j.nuclphysbps.2013.04.033
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