Speaker
sunanda .
Description
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 way to figure out its energetics to produce neutrino. Several models on considering lepto -hardronic channels to produce the gamma rays and neutrino from this blazar has 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.
Keywords
AGNs, Neutrinos, Gamma rays
| Subcategory | Theoretical Results |
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Primary authors
sunanda .
Dr
Reetanjali Moharana
(IIT Jodhpur)
