Extragalactic Diffuse Cascade Emission as a Probe of Processes in Active Galactic Nuclei
Anna Vladimir Uryson1 Show affiliations
- P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Russia
Space Science International, Volume 5, Issue 1, pp. 1–6 · doi.org/10.3844/ajssp.2024.1.6
Abstract
In this study, we discuss possible imprint of source characteristics on extragalactic diffuse cascade emission that is initiated by ultra-high energy cosmic rays propagating through the universe. The common opinion is that cosmic ray sources are active galactic nuclei. Based on cascade emission analyses we demonstrate that possibly a new subclass of cosmic ray sources exists, a particle flux from which on the Earth is small, however producing noticeable gamma-ray and neutrino emissions in the universe. We also estimate a fraction of active galactic nuclei with super-strong magnetic fields in their centers among those with common characteristics.
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Uryson, A. V. (2024). Extragalactic Diffuse Cascade Emission as a Probe of Processes in Active Galactic Nuclei. Space Science International, 5(1), 1–6. https://doi.org/10.3844/ajssp.2024.1.6
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