Signatures of blazar spectra in the electromagnetic and hadronic intergalactic cascade models
- Авторы: Dzhatdoev T.A.1, Kircheva A.P.1,2, Lyukshin A.A.2, Khalikov E.V.1
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Учреждения:
- Skobeltsyn Institute of Nuclear Physics
- Faculty of Physics
- Выпуск: Том 81, № 4 (2017)
- Страницы: 443-445
- Раздел: 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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Аннотация
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).
Об авторах
T. Dzhatdoev
Skobeltsyn Institute of Nuclear Physics
Автор, ответственный за переписку.
Email: timur1606@gmail.com
Россия, Moscow, 119991
A. Kircheva
Skobeltsyn Institute of Nuclear Physics; Faculty of Physics
Email: timur1606@gmail.com
Россия, Moscow, 119991; Moscow, 119991
A. Lyukshin
Faculty of Physics
Email: timur1606@gmail.com
Россия, Moscow, 119991
E. Khalikov
Skobeltsyn Institute of Nuclear Physics
Email: timur1606@gmail.com
Россия, Moscow, 119991
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