On Gamma Rays as Predictors of Ultra-high-energy Cosmic-Ray Flux in Active Galactic Nuclei

Active galactic nuclei (AGN) are among the main candidates for ultra-high-energy cosmic-ray (UHECR) sources. However, while some theoretical and phenomenological works favor AGNs as the main sources, recent works have shown that using the very-high-energy γ -ray flux as a proxy for the UHECR flux le...

Полное описание

Библиографические подробности
Главные авторы: Cainã de Oliveira, Rodrigo Guedes Lang, Pedro Batista
Формат: Статья
Язык:English
Опубликовано: IOP Publishing 2025-01-01
Серии:The Astrophysical Journal
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Online-ссылка:https://doi.org/10.3847/1538-4357/adafa2