A flare in 2017 from TXS0506+056 has 3.5$\sigma$ 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 $\gamma -\gamma \rightarrow e^+e^-$ 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.
Modelling TXS0506+056 with internal $\gamma -\gamma$ secondaries
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Pre-published on:
July 31, 2021
Published on:
March 18, 2022
Abstract
DOI: https://doi.org/10.22323/1.395.1014
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.