A search for point sources of EeV neutrons
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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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The Pierre Auger Collaboration; Pastor Carpi, Sergio
Aquest document és un/a article, creat/da en: 2012
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.

    The Pierre Auger Collaboration Pastor Carpi, Sergio 2012 A search for point sources of EeV neutrons Astrophysical Journal 760 2 148-1 148-11
http://dx.doi.org/10.1088/0004-637X/760/2/148
distribuït sota llicència Creative Commons de Reconeixement-NoComercial 3.0 No adaptada

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