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Upper limits on the cosmic-ray luminosity of supernovae in nearby galaxies

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    0566030 - FZÚ 2023 RIV IT eng C - Conference Paper (international conference)
    Sasse, R. … Total 2 authors
    Upper limits on the cosmic-ray luminosity of supernovae in nearby galaxies.
    Proceedings of Science. Vol. 395. Trieste: Sissa Medilab srl, 2022, č. článku 461. ISSN 1824-8039.
    [International Cosmic Ray Conference /37./. Berlin (DE), 12.07.2021-23.07.2021]
    Research Infrastructure: AUGER-CZ II - 90102
    Keywords : cosmic microwave background * extragalactic background light
    OECD category: Particles and field physics
    https://pos.sissa.it/395/461

    Interactions between cosmic rays and also between cosmic rays and particles of the Cosmic Microwave Background and the Extragalactic Background Light produce charged and neutral pions. The mechanisms that can produce gamma-ray fluxes associated with cosmic rays are the decay of neutral pions, bremsstrahlung, and inverse Compton scattering from pions. These cascading processes show a correlation between the upper limit on the integral GeV-TeV gamma-ray flux and the upper limit on the UHECR luminosity, motivating the study of the multi-messengers to calculate luminosities of UHECRs for specific point sources.

    Permanent Link: https://hdl.handle.net/11104/0337472

     
     
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