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Recent astronomical observations reveal that Active Galactic Nuclei (AGN) aresources of high-energy radiation. For example, the Fermi-LAT and Hesstelescopes have detected gamma-ray emissions from the cores of several types ofAGN's. Even more, the Pierre Auger observatory has found a correlation ofultra-high energy cosmic ray events with the position of Active GalacticNuclei, such as Centaurus A. In this way, according to particle physics, a fluxof high-energy neutrinos should be expected from the interactions of cosmic andgamma-rays with the ambient matter and radiation at the source. In this work,estimations of the diffuse neutrino flux from AGN's arising from interactionsof the gamma radiation with the gas and dust of the sources will be presented.

High-energy neutrino production from photo-hadronic interactions of gamma rays from Active Galactic Nuclei at source