Lepto-hadronic $\gamma$-ray and neutrino emission from the jet of TXS 0506+056
N. Sahakyan

TL;DR
This paper models the lepto-hadronic processes in the blazar TXS 0506+056 to explain simultaneous gamma-ray and neutrino emissions, estimating proton energies, neutrino rates, and jet energetics based on observational data.
Contribution
It presents a lepto-hadronic emission model for TXS 0506+056 that accounts for observed gamma-ray and neutrino signals, with detailed energy and flux estimates.
Findings
Proton energy distribution follows ~E_p^{-2.50} up to 10 PeV.
Expected neutrino rate is approximately 0.46 events during active phases.
Proton injection luminosity exceeds 10^48 erg/s, much higher than electron luminosity.
Abstract
The observation of IceCube-170922A event from the direction of TXS 0506+056 when it was in its enhanced -ray emission state offers a unique opportunity to investigate the lepto-hadronic processes in blazar jets. Here, the observed broadband emission of TXS 0506+056 is explained by boosted synchrotron/synchrotron self Compton emission from the jet whereas the -ray data observed during the neutrino emission- by inelastic interactions of the jet-accelerated protons in a dense gaseous target. The proton energy distribution is , calculated straightforwardly from the data obtained by Fermi-LAT and MAGIC and if such distribution continues up to PeV, the expected neutrino rate is as high as events during the long active phase of the source or if the activity lasts 60 days. In this interpretation, the energy content of the…
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