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Research Article · Open access · Published 25 February 2024

Extragalactic Diffuse Cascade Emission as a Probe of Processes in Active Galactic Nuclei

Anna Vladimir Uryson1

Space Science International, Volume 5, Issue 1, pp. 1–6 · doi.org/10.3844/ajssp.2024.1.6

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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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Open access. This article is licensed under a Creative Commons Attribution 4.0 International Licence (CC BY 4.0), as printed on the article, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original authors and the source. No permission is needed.

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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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Extragalactic Diffuse Cascade Emission as a Probe of Processes in Active Galactic NucleiSpace Science International · Volume 5, Issue 1 · pp. 1–6 · CC BY 4.0Download