A search for point sources of EeV neutrons

Autores
Abreu, P.; Aglietta, M.; Ahlers, M.; Ahn, E. J.; Albuquerque, I. F. M.; Gomez Berisso, Mariano; Zhou, J.; Zhu, Y.; Zimbres Silva, M.; Ziolkowski, M.
Año de publicación
2012
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
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 (1018 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.
Fil: Abreu, P.. Technical University of Lisbon; Portugal
Fil: Aglietta, M.. Università di Torino; Italia
Fil: Ahlers, M.. University of Wisconsin; Estados Unidos
Fil: Ahn, E. J.. Fermi National Accelerator Laboratory; Estados Unidos
Fil: Albuquerque, I. F. M.. Universidade de Sao Paulo; Brasil
Fil: Gomez Berisso, Mariano. Comisión Nacional de Energía Atómica. Gerencia de Área de Investigaciones y Aplicaciones No Nucleares. Gerencia de Física (CAB); Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Zhou, J.. University of Chicago; Estados Unidos
Fil: Zhu, Y.. North­Institut für Prozessdatenverarbeitung und Elektronik; Alemania
Fil: Zimbres Silva, M.. Universidade Estadual de Campinas; Brasil. NYU Abu Dhabi; Emiratos Arabes Unidos
Fil: Ziolkowski, M.. Universitat Siegen; Alemania
Materia
COSMIC RAYS
GALAXY: DISK
METHODS: DATA ANALYSIS
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/217973

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spelling A search for point sources of EeV neutronsAbreu, P.Aglietta, M.Ahlers, M.Ahn, E. J.Albuquerque, I. F. M.Gomez Berisso, MarianoZhou, J.Zhu, Y.Zimbres Silva, M.Ziolkowski, M.COSMIC RAYSGALAXY: DISKMETHODS: DATA ANALYSIShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1A 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 (1018 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.Fil: Abreu, P.. Technical University of Lisbon; PortugalFil: Aglietta, M.. Università di Torino; ItaliaFil: Ahlers, M.. University of Wisconsin; Estados UnidosFil: Ahn, E. J.. Fermi National Accelerator Laboratory; Estados UnidosFil: Albuquerque, I. F. M.. Universidade de Sao Paulo; BrasilFil: Gomez Berisso, Mariano. Comisión Nacional de Energía Atómica. Gerencia de Área de Investigaciones y Aplicaciones No Nucleares. Gerencia de Física (CAB); Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Zhou, J.. University of Chicago; Estados UnidosFil: Zhu, Y.. North­Institut für Prozessdatenverarbeitung und Elektronik; AlemaniaFil: Zimbres Silva, M.. Universidade Estadual de Campinas; Brasil. NYU Abu Dhabi; Emiratos Arabes UnidosFil: Ziolkowski, M.. Universitat Siegen; AlemaniaIOP Publishing2012-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/217973Abreu, P.; Aglietta, M.; Ahlers, M.; Ahn, E. J.; Albuquerque, I. F. M.; et al.; A search for point sources of EeV neutrons; IOP Publishing; Astrophysical Journal; 760; 2; 12-2012; 148-1490004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/760/2/148info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/0004-637X/760/2/148info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:05:28Zoai:ri.conicet.gov.ar:11336/217973instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:05:28.397CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv A search for point sources of EeV neutrons
title A search for point sources of EeV neutrons
spellingShingle A search for point sources of EeV neutrons
Abreu, P.
COSMIC RAYS
GALAXY: DISK
METHODS: DATA ANALYSIS
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 A search for point sources of EeV neutrons
dc.creator.none.fl_str_mv Abreu, P.
Aglietta, M.
Ahlers, M.
Ahn, E. J.
Albuquerque, I. F. M.
Gomez Berisso, Mariano
Zhou, J.
Zhu, Y.
Zimbres Silva, M.
Ziolkowski, M.
author Abreu, P.
author_facet Abreu, P.
Aglietta, M.
Ahlers, M.
Ahn, E. J.
Albuquerque, I. F. M.
Gomez Berisso, Mariano
Zhou, J.
Zhu, Y.
Zimbres Silva, M.
Ziolkowski, M.
author_role author
author2 Aglietta, M.
Ahlers, M.
Ahn, E. J.
Albuquerque, I. F. M.
Gomez Berisso, Mariano
Zhou, J.
Zhu, Y.
Zimbres Silva, M.
Ziolkowski, M.
author2_role author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv COSMIC RAYS
GALAXY: DISK
METHODS: DATA ANALYSIS
topic COSMIC RAYS
GALAXY: DISK
METHODS: DATA ANALYSIS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv 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 (1018 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.
Fil: Abreu, P.. Technical University of Lisbon; Portugal
Fil: Aglietta, M.. Università di Torino; Italia
Fil: Ahlers, M.. University of Wisconsin; Estados Unidos
Fil: Ahn, E. J.. Fermi National Accelerator Laboratory; Estados Unidos
Fil: Albuquerque, I. F. M.. Universidade de Sao Paulo; Brasil
Fil: Gomez Berisso, Mariano. Comisión Nacional de Energía Atómica. Gerencia de Área de Investigaciones y Aplicaciones No Nucleares. Gerencia de Física (CAB); Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Zhou, J.. University of Chicago; Estados Unidos
Fil: Zhu, Y.. North­Institut für Prozessdatenverarbeitung und Elektronik; Alemania
Fil: Zimbres Silva, M.. Universidade Estadual de Campinas; Brasil. NYU Abu Dhabi; Emiratos Arabes Unidos
Fil: Ziolkowski, M.. Universitat Siegen; Alemania
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 (1018 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.
publishDate 2012
dc.date.none.fl_str_mv 2012-12
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/217973
Abreu, P.; Aglietta, M.; Ahlers, M.; Ahn, E. J.; Albuquerque, I. F. M.; et al.; A search for point sources of EeV neutrons; IOP Publishing; Astrophysical Journal; 760; 2; 12-2012; 148-149
0004-637X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/217973
identifier_str_mv Abreu, P.; Aglietta, M.; Ahlers, M.; Ahn, E. J.; Albuquerque, I. F. M.; et al.; A search for point sources of EeV neutrons; IOP Publishing; Astrophysical Journal; 760; 2; 12-2012; 148-149
0004-637X
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/760/2/148
info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/0004-637X/760/2/148
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
application/pdf
dc.publisher.none.fl_str_mv IOP Publishing
publisher.none.fl_str_mv IOP Publishing
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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