13-16 February 2012
CERN
Europe/Zurich timezone
- conf@2012.uhecr.org
Contact
Search for ultra-high energy neutrinos at the Pierre Auger Observatory
Presented by Sergio NAVAS CONCHA
Type: poster
Content
The Pierre Auger Observatory has the capability of detecting ultra-high
energy neutrinos of all flavours. They interact through charged and
neutral currents in the atmosphere (downward-going) and through the
``Earth-skimming'' mechanism (upward-going). The main challenge in
detecting ultra-high energy neutrinos with the Pierre Auger Observatory
is to identify a neutrino-induced shower in the overwhelming background
of showers initiated by ultra-high energy cosmic rays, possibly protons,
heavy nuclei or even photons. The neutrino search analyses and the
most up-to-date upper limits on the neutrino fluxes are reported.
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