limit on uhe neutrino fluxes from the pierre auger observatory

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ID: 229555
2013
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Abstract
The surface detector of the Pierre Auger Observatory is sensitive to Ultra High Energy (UHE) neutrinos. Neutrinos of all flavors can interact in the atmosphere producing inclined showers near the ground. Moreover, ultra high energy Earth-skimming tau neutrinos can be observed through the detection of showers induced by the decay of tau leptons created by interactions in the Earth’s crust. In both cases, neutrino showers can be identified through the time structure of the signals in the surface detector stations. Two sets of identification criteria have been designed to search for down-going and up-going neutrinos in the recorded data, with no candidates found. We will discuss the identification criteria used, and we will present the corresponding limits on the diffuse and point source neutrino fluxes.
Reference Key
maldera2013actalimit Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors ;S. Maldera
Journal the journal of nutrition
Year 2013
DOI
10.14311/AP.2013.53.0756
URL
https://ojs.cvut.cz/ojs/index.php/ap/article/view/1974
Keywords
engineering (general) civil engineering (general)

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