Speaker
Luis Anchordoqui
(City University of New York)
Description
Cosmic neutrinos with energies near 10^9 GeV and above are detectable with the Surface Detector array of the Pierre Auger Observatory. We report here on searches through Auger data from 1 January 2004 until 20 June 2013. No neutrino candidates were found, yielding a limit to the diffuse flux of ultra-high energy neutrinos that challenges the Waxman-Bahcall benchmark predictions.
Authors
Luis Anchordoqui
(City University of New York)
Pierre Auger Collaboration
(Av. San Mart ́ın Norte 306, 5613 Malargu ̈e, Mendoza, Argentina)
