Mostrar el registro sencillo del ítem

dc.contributor.author
Abreu, P.  
dc.contributor.author
Aglietta, M.  
dc.contributor.author
Ahlers, M.  
dc.contributor.author
Ahn, E. J.  
dc.contributor.author
Albuquerque, I. F. M.  
dc.contributor.author
Gomez Berisso, Mariano  
dc.contributor.author
Zhou, J.  
dc.contributor.author
Zhu, Y.  
dc.contributor.author
Zimbres Silva, M.  
dc.contributor.author
Ziolkowski, M.  
dc.date.available
2023-11-14T10:37:57Z  
dc.date.issued
2012-12  
dc.identifier.citation
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  
dc.identifier.issn
0004-637X  
dc.identifier.uri
http://hdl.handle.net/11336/217973  
dc.description.abstract
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.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
IOP Publishing  
dc.rights
info:eu-repo/semantics/openAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
COSMIC RAYS  
dc.subject
GALAXY: DISK  
dc.subject
METHODS: DATA ANALYSIS  
dc.subject.classification
Física de Partículas y Campos  
dc.subject.classification
Ciencias Físicas  
dc.subject.classification
CIENCIAS NATURALES Y EXACTAS  
dc.title
A search for point sources of EeV neutrons  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2023-02-26T15:33:25Z  
dc.journal.volume
760  
dc.journal.number
2  
dc.journal.pagination
148-149  
dc.journal.pais
Reino Unido  
dc.journal.ciudad
Londres  
dc.description.fil
Fil: Abreu, P.. Technical University of Lisbon; Portugal  
dc.description.fil
Fil: Aglietta, M.. Università di Torino; Italia  
dc.description.fil
Fil: Ahlers, M.. University of Wisconsin; Estados Unidos  
dc.description.fil
Fil: Ahn, E. J.. Fermi National Accelerator Laboratory; Estados Unidos  
dc.description.fil
Fil: Albuquerque, I. F. M.. Universidade de Sao Paulo; Brasil  
dc.description.fil
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  
dc.description.fil
Fil: Zhou, J.. University of Chicago; Estados Unidos  
dc.description.fil
Fil: Zhu, Y.. North­Institut für Prozessdatenverarbeitung und Elektronik; Alemania  
dc.description.fil
Fil: Zimbres Silva, M.. Universidade Estadual de Campinas; Brasil. NYU Abu Dhabi; Emiratos Arabes Unidos  
dc.description.fil
Fil: Ziolkowski, M.. Universitat Siegen; Alemania  
dc.journal.title
Astrophysical Journal  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/https://doi.org/10.1088/0004-637X/760/2/148  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/0004-637X/760/2/148  

Archivos asociados
Thumbnail
 
Tamaño: 1.693Mb
Formato: PDF
.