Signatures of blazar spectra in the electromagnetic and hadronic intergalactic cascade models


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Resumo

There are indications that a secondary component of cascade photons is present in the spectra of some bright blazars. The main spectral signatures are considered using the electromagnetic model. The simplest version of the hadronic cascade model can be distinguished from the electromagnetic cascade at a significance level of ~3 σ for a typical observation of a blazar at the Cherenkov Telescope Array (CTA).

Sobre autores

T. Dzhatdoev

Skobeltsyn Institute of Nuclear Physics

Autor responsável pela correspondência
Email: timur1606@gmail.com
Rússia, Moscow, 119991

A. Kircheva

Skobeltsyn Institute of Nuclear Physics; Faculty of Physics

Email: timur1606@gmail.com
Rússia, Moscow, 119991; Moscow, 119991

A. Lyukshin

Faculty of Physics

Email: timur1606@gmail.com
Rússia, Moscow, 119991

E. Khalikov

Skobeltsyn Institute of Nuclear Physics

Email: timur1606@gmail.com
Rússia, Moscow, 119991

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