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

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The Pierre Auger Collaboration; Pastor Carpi, Sergio
Aquest document és un/a article, creat/da en: 2012
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.

    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
http://dx.doi.org/10.1016/j.nima.2010.11.014
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