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Hadronic modeling of TeV AGN: gammas and neutrinos · Around

2016

Hadronic modeling of TeV AGN: gammas and neutrinos

Cerruti, M., Zech, A., Emery, G. et al.

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Blazar emission models are usually divided into two big families, leptonic and hadronic, according to the particles which are responsible for the gamma-ray component of their spectral energy distributions.

Even though leptonic models have been successful in explaining the gamma-ray emission from most blazars, hadronic models still present an intriguing alternative.
They have the unique advantage to link the emission of photons, neutrinos, and cosmic rays from the astrophysical source.
We have developed a stationary one-zone lepto-hadronic code to model the emission from blazars in both leptonic and hadronic scenarios.

Built on

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Then

P. Padovani and E. Resconi, MNRAS 443
2014
Later among the works it cites.
M. Cerruti, A. Zech, C. Boisson, and S. Inoue, MNRAS 448
2015
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M. Petropoulou, S. Dimitrakoudis, P. Padovani, and et al., MNRAS 448
2015
Later among the works it cites.
A. M. Brown, C. Boehm, J. Graham, T. Lacroix, P. M. Chadwick, and J. Silk, ArXiv e-prints (2016), arXiv:1603.05469 [astro-ph.HE]
Original
2016
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