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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/217973
Ver los metadatos del registro completo
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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 |
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CONICET Digital (CONICET) |
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CONICET Digital (CONICET) |
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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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13.070432 |