A Targeted Search for Point Sources of EeV Neutrons

Abstract

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.

arXiv comment17 pages, accepted for publication in The Astrophysical Journal Letters

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Cited by in corpus (10)

• The Pierre Auger Cosmic Ray Observatory
• Ultra-High-Energy Cosmic Rays: The Intersection of the Cosmic and Energy Frontiers
• Multi-Messenger Physics with the Pierre Auger Observatory
• A targeted search for point sources of EeV photons with the Pierre Auger Observatory
• Russian-German Astroparticle Data Life Cycle Initiative
• Search for Sources of High Energy Neutrons with Four Years of Data from the IceTop Detector
• Ultra-High Energy Cosmic Rays: Recent Results and Future Plans of Auger
• Report from the Multi-Messenger Working Group at UHECR-2014 Conference
• Search for Ultra-High Energy Photons with the Pierre Auger Observatory
• Data Processing at the Pierre Auger Observatory