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SUMMARY:The Search for Ultra-High Energy Neutrinos through Highly Inclined
  Air Showers in the Pierre Auger Observatory
DTSTART;VALUE=DATE-TIME:20210901T154500Z
DTEND;VALUE=DATE-TIME:20210901T160000Z
DTSTAMP;VALUE=DATE-TIME:20260312T200558Z
UID:indico-contribution-15764@indico.ific.uv.es
DESCRIPTION:Speakers: Gonzalo Parente (Universidade de Santiago de Compost
 ela)\nThe Surface Detector of the Pierre Auger Observatory\, an array of 1
 600 water-\nCherenkov stations in a triangular grid with 1500 m separation
  between\nstations\, has the capability to detect neutrinos with energy ab
 ove 10^17 eV. The\nidentification through the special characteristics of h
 ighly inclined showers is\nefficiently performed for neutrinos of all flav
 ours interacting deep in the\natmosphere at large zenith angles as well as
  for Earth skimming τ neutrinos.\nIn this talk I review the status of the
  neutrino search at the Observatory using\nabout 15 years of data. Restric
 tive upper bounds on the neutrino flux from\ndiffuse sources and from poin
 t-like steady sources were stablished placing\nstrong constraints on sever
 al models of neutrino production at EeV energies\nand on the properties of
  the sources of ultra-high-energy cosmic rays.\nUnrivaled sensitivity in s
 earches for transient sources has been also achieved.\n\nhttps://indico.if
 ic.uv.es/event/6178/contributions/15764/
LOCATION:
URL:https://indico.ific.uv.es/event/6178/contributions/15764/
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