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Accès ouvert déclaré 2014 article

A Targeted Search for Point Sources of EeV Neutrons

12Citations signalées, ce qui n’est pas une note de qualité
104Institutions déclarées
18Pays d’affiliation déclarés

Rattachement africain : de, pt, it, us, fr, br, ar, mx, es, nl, ro, au, cz, pl, vn, si, gb, hr. Niveau de preuve : code pays fourni par la source.

Le résumé fourni par la source

A flux of neutrons from an astrophysical source in the Galaxy can be detected in the Pierre Auger Observatory as an excess of cosmic-ray air showers arriving from the direction of the source. To avoid the statistical penalty for making many trials, classes of objects are tested in combinations as nine "target sets," in addition to the search for a neutron flux from the Galactic center or from the Galactic plane. Within a target set, each candidate source is weighted in proportion to its electromagnetic flux, its exposure to the Auger Observatory, and its flux attenuation factor due to neutron decay. These searches do not find evidence for a neutron flux from any class of candidate sources. Tabulated results give the combined p-value for each class, with and without the weights, and also the flux upper limit for the most significant candidate source within each class. These limits on fluxes of neutrons significantly constrain models of EeV proton emission from non-transient discrete sources in the Galaxy. © 2014. The American Astronomical Society. All rights reserved..

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Le contrôle bibliographique ouvert

Aucun DOI disponible pour le contrôle Crossref.

Les institutions déclarées

University of SiegenUniversity of LisbonLIP - Laboratory of Instrumentation and Experimental Particle PhysicsOsservatorio Astrofisico di TorinoUniversity of Wisconsin–MadisonFermi National Accelerator LaboratoryCentre National de la Recherche ScientifiqueUniversité Paris-SaclayInstitut de PhysiqueInstitut National de Physique Nucléaire et de Physique des ParticulesUniversidade de São PauloConsejo Nacional de Investigaciones Científicas y TécnicasBalseiro InstituteBariloche Atomic CentreNew York UniversityThe Ohio State UniversityNational Technological UniversityNational University of General San MartínInstituto de Tecnologías en Detección y AstropartículasUniversidad Nacional Autónoma de MéxicoUniversidade de Santiago de CompostelaUniversität HamburgIstituto Nazionale di Fisica Nucleare, Sezione di NapoliRadboud University NijmegenUniversity of Wisconsin–MilwaukeeUniversidad Complutense de MadridUniversité Paris CitéSorbonne UniversitéLaboratoire de Physique Nucléaire et de Hautes ÉnergiesLaboratoire de Physique Subatomique et de CosmologieUniversité Grenoble AlpesComisión Nacional de Energía AtómicaUniversitatea Națională de Știință și Tehnologie Politehnica BucureștiThe University of AdelaideKarlsruhe Institute of TechnologyUniversity of WuppertalMax Planck Institute for Radio AstronomyCzech Academy of SciencesFZU ‒ Institute of Physics of the Academy of Sciences of the Czech RepublicIstituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran SassoUniversidade Federal do Rio de JaneiroInstitute of Nuclear Physics, Polish Academy of SciencesColorado State UniversityHoria Hulubei National Institute for R and D in Physics and Nuclear EngineeringColorado State University PuebloUniversidad de GranadaPennsylvania State UniversityCentro de Investigación y de Estudios Avanzados del Instituto Politécnico NacionalIstituto Nazionale di Fisica Nucleare, Sezione di MilanoIstituto Nazionale di Fisica Nucleare, Sezione di Roma IIstituto Nazionale di Fisica Nucleare, Sezione di CataniaUniversity of SalentoIstituto Nazionale di Fisica Nucleare, Sezione di LecceIstituto Nazionale di Fisica Nucleare, Sezione di TorinoUniversidad Michoacana de San Nicolás de HidalgoUniversidade Estadual de Campinas (UNICAMP)Pierre Auger ObservatoryCase Western Reserve UniversityUniversity of ChicagoObservatoire de ParisLaboratoire de Physique Subatomique et des Technologies AssociéesNantes UniversitéUniversidad de Buenos AiresInstitute of Astronomy and Space PhysicsUniversidade Federal FluminenseNational Institute for Subatomic PhysicsUniversidad de AlcaláMichigan Technological UniversityUniversity of L'AquilaInstitute for Nuclear Science and TechnologyUniversity of GroningenUniversidad Nacional de La PlataRWTH Aachen UniversityNetherlands Institute for Radio AstronomyUniversity of Nova GoricaJožef Stefan InstituteUniversity of Hawaiʻi at MānoaUniversity of Hawaii SystemUniversity of ŁódźUniversidade Estadual de Feira de SantanaPalacký University OlomoucInstitute of Space Science - INFLPR SubsidiaryLouisiana State UniversityIstituto di Astrofisica Spaziale e Fisica cosmica di PalermoUniversity of New MexicoEscola Bahiana de Medicina e Saúde PúblicaUniversidade Federal do ABCBenemérita Universidad Autónoma de PueblaUniversity of LeedsCentro Brasileiro de Pesquisas FísicasColorado School of MinesRuđer Bošković InstituteInstitute of Physics RosarioUniversidade Federal de PelotasCharles UniversityInstitute of Scientific and Technical Research for DefenseUniversitat de ValènciaUniversidade Federal da BahiaIstituto Nazionale di Fisica Nucleare, Sezione di GenovaUniversity of Nebraska–LincolnGran Sasso Science InstituteUniversity of BucharestNortheastern UniversityLos Alamos National Laboratory

Une affiliation ne permet pas de déduire la nationalité d’un auteur.

Les sujets associés

Astrophysics and Cosmic PhenomenaDark Matter and Cosmic PhenomenaNeutrino Physics Research

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