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Volume 395 - 37th International Cosmic Ray Conference (ICRC2021) - MM - Multi-Messenger
Modelling TXS0506+056 with internal γ−γ secondaries
 Sunanda* and R. Moharana
*: corresponding author
Full text: pdf
Pre-published on: July 31, 2021
Published on: March 18, 2022
Abstract
A flare in 2017 from TXS0506+056 has 3.5σ spatial as well as temporal correlation with IceCube-170922A neutrino event above energy 290 TeV. The multi-wavelength modeling of the source is one of the viable ways to figure out its energetics to produce neutrino. Several models on considering lepto -hadronic channels to produce the gamma rays and neutrino from this blazar have already been done.
We report here the secondary contribution resulted from the γ−γ→e+e− interaction between self synchrotron (SSC) and synchrotron photon in the blazar TXS0506+056. This study would help in understanding the maximum energy of the electrons produced at the source.
DOI: https://doi.org/10.22323/1.395.1014
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