Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory

The Surface Detector of the Pierre Auger Observatory is sensitive to neutrinos of all flavors above 0.1 EeV. These interact through charged and neutral currents in the atmosphere giving rise to extensive air showers. When interacting deeply in the atmosphere at nearly horizontal incidence, neutrinos...

Descripción completa

Detalles Bibliográficos
Publicado: 2011
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_15507998_v84_n12_p_Multitudinario
http://hdl.handle.net/20.500.12110/paper_15507998_v84_n12_p_Multitudinario
Aporte de:
id paper:paper_15507998_v84_n12_p_Multitudinario
record_format dspace
spelling paper:paper_15507998_v84_n12_p_Multitudinario2023-06-08T16:22:21Z Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory The Surface Detector of the Pierre Auger Observatory is sensitive to neutrinos of all flavors above 0.1 EeV. These interact through charged and neutral currents in the atmosphere giving rise to extensive air showers. When interacting deeply in the atmosphere at nearly horizontal incidence, neutrinos can be distinguished from regular hadronic cosmic rays by the broad time structure of their shower signals in the water-Cherenkov detectors. In this paper we present for the first time an analysis based on down-going neutrinos. We describe the search procedure, the possible sources of background, the method to compute the exposure and the associated systematic uncertainties. No candidate neutrinos have been found in data collected from 1 January 2004 to 31 May 2010. Assuming an E - 2 differential energy spectrum the limit on the single-flavor neutrino is E2dN/dE<1.74×10 - 7GeVcm - 2s - 1sr - 1 at 90% C.L. in the energy range 1×1017eV<E<1×1020eV. © 2011 American Physical Society. 2011 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_15507998_v84_n12_p_Multitudinario http://hdl.handle.net/20.500.12110/paper_15507998_v84_n12_p_Multitudinario
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
description The Surface Detector of the Pierre Auger Observatory is sensitive to neutrinos of all flavors above 0.1 EeV. These interact through charged and neutral currents in the atmosphere giving rise to extensive air showers. When interacting deeply in the atmosphere at nearly horizontal incidence, neutrinos can be distinguished from regular hadronic cosmic rays by the broad time structure of their shower signals in the water-Cherenkov detectors. In this paper we present for the first time an analysis based on down-going neutrinos. We describe the search procedure, the possible sources of background, the method to compute the exposure and the associated systematic uncertainties. No candidate neutrinos have been found in data collected from 1 January 2004 to 31 May 2010. Assuming an E - 2 differential energy spectrum the limit on the single-flavor neutrino is E2dN/dE<1.74×10 - 7GeVcm - 2s - 1sr - 1 at 90% C.L. in the energy range 1×1017eV<E<1×1020eV. © 2011 American Physical Society.
title Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory
spellingShingle Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory
title_short Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory
title_full Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory
title_fullStr Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory
title_full_unstemmed Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory
title_sort search for ultrahigh energy neutrinos in highly inclined events at the pierre auger observatory
publishDate 2011
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_15507998_v84_n12_p_Multitudinario
http://hdl.handle.net/20.500.12110/paper_15507998_v84_n12_p_Multitudinario
_version_ 1768542806049030144