Upper Limit on the Diffuse Flux of Ultrahigh Energy Tau Neutrinos from the Pierre Auger Observatory
The surface detector array of the Pierre Auger Observatory is sensitive to Earth-skimming tau neutrinos that interact in Earth's crust. Tau leptons from ντ charged-current interactions can emerge and decay in the atmosphere to produce a nearly horizontal shower with a significant electromagneti...
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Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00319007_v100_n21_p_Multitudinario |
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todo:paper_00319007_v100_n21_p_Multitudinario2023-10-03T14:41:58Z Upper Limit on the Diffuse Flux of Ultrahigh Energy Tau Neutrinos from the Pierre Auger Observatory Multitudinario:453 Earth (planet) Electromagnetism Space research Diffuse Flux Pierre Auger Observatory High energy physics The surface detector array of the Pierre Auger Observatory is sensitive to Earth-skimming tau neutrinos that interact in Earth's crust. Tau leptons from ντ charged-current interactions can emerge and decay in the atmosphere to produce a nearly horizontal shower with a significant electromagnetic component. The data collected between 1 January2004 and 31 August 2007 are used to place an upper limit on the diffuse flux of ντ at EeV energies. Assuming an Eν-2 differential energy spectrum the limit set at 90% C.L. is Eν2dNντ/dEν<1.3×10-7GeVcm-2s-1sr-1 in the energy range 2×1017eV<Eν<2×1019eV. © 2008 The American Physical Society. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00319007_v100_n21_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) |
topic |
Earth (planet) Electromagnetism Space research Diffuse Flux Pierre Auger Observatory High energy physics |
spellingShingle |
Earth (planet) Electromagnetism Space research Diffuse Flux Pierre Auger Observatory High energy physics Multitudinario:453 Upper Limit on the Diffuse Flux of Ultrahigh Energy Tau Neutrinos from the Pierre Auger Observatory |
topic_facet |
Earth (planet) Electromagnetism Space research Diffuse Flux Pierre Auger Observatory High energy physics |
description |
The surface detector array of the Pierre Auger Observatory is sensitive to Earth-skimming tau neutrinos that interact in Earth's crust. Tau leptons from ντ charged-current interactions can emerge and decay in the atmosphere to produce a nearly horizontal shower with a significant electromagnetic component. The data collected between 1 January2004 and 31 August 2007 are used to place an upper limit on the diffuse flux of ντ at EeV energies. Assuming an Eν-2 differential energy spectrum the limit set at 90% C.L. is Eν2dNντ/dEν<1.3×10-7GeVcm-2s-1sr-1 in the energy range 2×1017eV<Eν<2×1019eV. © 2008 The American Physical Society. |
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JOUR |
author |
Multitudinario:453 |
author_facet |
Multitudinario:453 |
author_sort |
Multitudinario:453 |
title |
Upper Limit on the Diffuse Flux of Ultrahigh Energy Tau Neutrinos from the Pierre Auger Observatory |
title_short |
Upper Limit on the Diffuse Flux of Ultrahigh Energy Tau Neutrinos from the Pierre Auger Observatory |
title_full |
Upper Limit on the Diffuse Flux of Ultrahigh Energy Tau Neutrinos from the Pierre Auger Observatory |
title_fullStr |
Upper Limit on the Diffuse Flux of Ultrahigh Energy Tau Neutrinos from the Pierre Auger Observatory |
title_full_unstemmed |
Upper Limit on the Diffuse Flux of Ultrahigh Energy Tau Neutrinos from the Pierre Auger Observatory |
title_sort |
upper limit on the diffuse flux of ultrahigh energy tau neutrinos from the pierre auger observatory |
url |
http://hdl.handle.net/20.500.12110/paper_00319007_v100_n21_p_Multitudinario |
work_keys_str_mv |
AT multitudinario453 upperlimitonthediffusefluxofultrahighenergytauneutrinosfromthepierreaugerobservatory |
_version_ |
1807315642891632640 |