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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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 |
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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.. |
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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 AT multitudinario509 searchforpointsourcesofeevneutrons |
_version_ |
1807318725853970432 |