Signatures of blazar spectra in the electromagnetic and hadronic intergalactic cascade models
- 作者: Dzhatdoev T.A.1, Kircheva A.P.1,2, Lyukshin A.A.2, Khalikov E.V.1
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隶属关系:
- Skobeltsyn Institute of Nuclear Physics
- Faculty of Physics
- 期: 卷 81, 编号 4 (2017)
- 页面: 443-445
- 栏目: 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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详细
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).
作者简介
T. Dzhatdoev
Skobeltsyn Institute of Nuclear Physics
编辑信件的主要联系方式.
Email: timur1606@gmail.com
俄罗斯联邦, Moscow, 119991
A. Kircheva
Skobeltsyn Institute of Nuclear Physics; Faculty of Physics
Email: timur1606@gmail.com
俄罗斯联邦, Moscow, 119991; Moscow, 119991
A. Lyukshin
Faculty of Physics
Email: timur1606@gmail.com
俄罗斯联邦, Moscow, 119991
E. Khalikov
Skobeltsyn Institute of Nuclear Physics
Email: timur1606@gmail.com
俄罗斯联邦, Moscow, 119991
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