Diffuse CR, neutrino and gamma-ray fluxes from AGNs
Peer reviewed, Journal article
Published version
Permanent lenke
https://hdl.handle.net/11250/2648400Utgivelsesdato
2016Metadata
Vis full innførselSamlinger
- Institutt for fysikk [2702]
- Publikasjoner fra CRIStin - NTNU [38576]
Sammendrag
We investigate how the extragalactic proton component derived within the ’escape model’ canbe explained by astrophysical sources. We find that the complete extragalactic proton spectrumcan be explained by a single source population with late time evolution, such as BL Lacs orFR I galaxies. We then calculate the diffuse neutrino andg-ray fluxes produced by these CRprotons interacting with gas inside their sources, their host galaxies and galaxy clusters. For aspectral slope of CRs close toa=2:1