A search for point sources of EeV neutrons

A thorough search of the sky exposed at the Pierre Auger Cosmic Ray Observatory reveals no statistically significant excess of events in any small solid angle that would be indicative of a flux of neutral particles from a discrete source. The search covers from -90° to +15° in declination using four...

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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_0004637X_v760_n2_p_Multitudinario
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spelling todo:paper_0004637X_v760_n2_p_Multitudinario2023-10-03T14:02:30Z A search for point sources of EeV neutrons Multitudinario:509 cosmic rays Galaxy: disk methods: data analysis A thorough search of the sky exposed at the Pierre Auger Cosmic Ray Observatory reveals no statistically significant excess of events in any small solid angle that would be indicative of a flux of neutral particles from a discrete source. The search covers from -90° to +15° in declination using four different energy ranges above 1 EeV (10 18 eV). The method used in this search is more sensitive to neutrons than to photons. The upper limit on a neutron flux is derived for a dense grid of directions for each of the four energy ranges. These results constrain scenarios for the production of ultrahigh energy cosmic rays in the Galaxy. © 2012. The American Astronomical Society. All rights reserved.. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_0004637X_v760_n2_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 cosmic rays
Galaxy: disk
methods: data analysis
spellingShingle cosmic rays
Galaxy: disk
methods: data analysis
Multitudinario:509
A search for point sources of EeV neutrons
topic_facet cosmic rays
Galaxy: disk
methods: data analysis
description A thorough search of the sky exposed at the Pierre Auger Cosmic Ray Observatory reveals no statistically significant excess of events in any small solid angle that would be indicative of a flux of neutral particles from a discrete source. The search covers from -90° to +15° in declination using four different energy ranges above 1 EeV (10 18 eV). The method used in this search is more sensitive to neutrons than to photons. The upper limit on a neutron flux is derived for a dense grid of directions for each of the four energy ranges. These results constrain scenarios for the production of ultrahigh energy cosmic rays in the Galaxy. © 2012. The American Astronomical Society. All rights reserved..
format JOUR
author Multitudinario:509
author_facet Multitudinario:509
author_sort Multitudinario:509
title A search for point sources of EeV neutrons
title_short A search for point sources of EeV neutrons
title_full A search for point sources of EeV neutrons
title_fullStr A search for point sources of EeV neutrons
title_full_unstemmed A search for point sources of EeV neutrons
title_sort search for point sources of eev neutrons
url http://hdl.handle.net/20.500.12110/paper_0004637X_v760_n2_p_Multitudinario
work_keys_str_mv AT multitudinario509 asearchforpointsourcesofeevneutrons
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