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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Publicado: 2012
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Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v760_n2_p_Multitudinario
http://hdl.handle.net/20.500.12110/paper_0004637X_v760_n2_p_Multitudinario
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spelling paper:paper_0004637X_v760_n2_p_Multitudinario2023-06-08T14:29:09Z A search for point sources of EeV neutrons 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.. 2012 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v760_n2_p_Multitudinario 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
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..
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
publishDate 2012
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v760_n2_p_Multitudinario
http://hdl.handle.net/20.500.12110/paper_0004637X_v760_n2_p_Multitudinario
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