Signatures of blazar spectra in the electromagnetic and hadronic intergalactic cascade models
- Autores: Dzhatdoev T.A.1, Kircheva A.P.1,2, Lyukshin A.A.2, Khalikov E.V.1
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Afiliações:
- Skobeltsyn Institute of Nuclear Physics
- Faculty of Physics
- Edição: Volume 81, Nº 4 (2017)
- Páginas: 443-445
- Seção: Proceedings of the 34th National Conference on Cosmic Rays
- URL: https://journals.rcsi.science/1062-8738/article/view/185037
- DOI: https://doi.org/10.3103/S1062873817040165
- ID: 185037
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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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