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A TARGETED SEARCH FOR POINT SOURCES OF EeV NEUTRONS

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F14%3A10283724" target="_blank" >RIV/00216208:11320/14:10283724 - isvavai.cz</a>

  • Alternative codes found

    RIV/68378271:_____/14:00436598 RIV/61989592:15310/14:33151045

  • Result on the web

    <a href="http://dx.doi.org/10.1088/2041-8205/789/2/L34" target="_blank" >http://dx.doi.org/10.1088/2041-8205/789/2/L34</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1088/2041-8205/789/2/L34" target="_blank" >10.1088/2041-8205/789/2/L34</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    A TARGETED SEARCH FOR POINT SOURCES OF EeV NEUTRONS

  • Original language description

    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 electromagneticflux, 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 sou

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BF - Elementary particle theory and high energy physics

  • OECD FORD branch

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2014

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Astrophysical Journal Letters

  • ISSN

    2041-8205

  • e-ISSN

  • Volume of the periodical

    789

  • Issue of the periodical within the volume

    2

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    7

  • Pages from-to

  • UT code for WoS article

    000339876800009

  • EID of the result in the Scopus database