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A search for point sources of EeV neutrons

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A search for point sources of EeV neutrons

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dc.contributor.author The Pierre Auger Collaboration
dc.contributor.author Pastor Carpi, Sergio
dc.date.accessioned 2015-10-29T11:09:39Z
dc.date.available 2015-10-29T11:09:39Z
dc.date.issued 2012
dc.identifier.citation The Pierre Auger Collaboration Pastor Carpi, Sergio 2012 A search for point sources of EeV neutrons Astrophysical Journal 760 2 148-1 148-11
dc.identifier.uri http://hdl.handle.net/10550/47946
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 degrees to +15 degrees 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.
dc.language.iso eng
dc.relation.ispartof Astrophysical Journal, 2012, vol. 760, num. 2, p. 148-1-148-11
dc.subject Física
dc.title A search for point sources of EeV neutrons
dc.type journal article es_ES
dc.date.updated 2015-10-29T11:09:40Z
dc.identifier.doi 10.1088/0004-637X/760/2/148
dc.identifier.idgrec 082471
dc.rights.accessRights open access es_ES

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