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Diffuse flux of ultra-high-energy photons from cosmic-ray interactions in the Disk of the Galaxy and implications for the search for decaying super-heavy dark matter

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F22%3A00564430" target="_blank" >RIV/68378271:_____/22:00564430 - isvavai.cz</a>

  • Result on the web

    <a href="https://hdl.handle.net/11104/0336104" target="_blank" >https://hdl.handle.net/11104/0336104</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.3847/1538-4357/ac5cbe" target="_blank" >10.3847/1538-4357/ac5cbe</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Diffuse flux of ultra-high-energy photons from cosmic-ray interactions in the Disk of the Galaxy and implications for the search for decaying super-heavy dark matter

  • Original language description

    An estimate of the expected photon flux above 10(17) eV from the interactions of ultra-high-energy cosmic rays with the matter in the Galactic disk is presented. Uncertainties arising from the distribution of the gas in the disk, the absolute level of the cosmic-ray flux, and the composition of the cosmic rays are taken into account. Within these uncertainties, the integrated photon flux above 10(17) eV is averaged out over Galactic latitude less than 5 degrees, between similar or equal to 3.2 x 10(-2) km(-2) yr(-1) sr(-1) and similar or equal to 8.7 x 10(-2) km(-2) yr(-1) sr(-1). The all-sky average value amounts to similar or equal to 1.1 x10(-2) km(-2) yr(-1) sr(-1) above 10(17) eV and decreases roughly as E (-2), making this diffuse flux the dominant one from cosmic-ray interactions for energy thresholds between 10(17) and 10(18) eV.n

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10303 - Particles and field physics

Result continuities

  • Project

  • Continuities

Others

  • Publication year

    2022

  • 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

  • ISSN

    0004-637X

  • e-ISSN

    1538-4357

  • Volume of the periodical

    929

  • Issue of the periodical within the volume

    1

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    8

  • Pages from-to

    55

  • UT code for WoS article

    000782189000001

  • EID of the result in the Scopus database

    2-s2.0-85129066537