Could TDE outflows produce the PeV neutrino events?

Abstract

A tidal disruption event (TDE), AT2019dsg, was observed to be associated with a PeV neutrino event, IceCube-191001A, lagging the optical outburst by a half year. It is known that TDEs may generate ultrafast outflows. If the TDE occurs in a cloudy environment, the outflow-cloud interactions may form shock waves which generate accelerated protons and hence delayed neutrinos from hadronic interactions in clouds. Here we investigate the neutrino production in AT2019dsg by examining the TDE outflow-cloud interaction model. We find that, for an outflow with a velocity of 0.07c and a kinetic luminosity of $10^{45}\mathrm{erg}{\mathrm{s}}^{-1}$, protons may be accelerated up to $\sim$ 60 PeV by the bow shocks, and generate PeV neutrinos by interactions with clouds. The predicted neutrino number in this model depends on the uncertainties of model parameters and in order to match the observations, some challenging values of parameters have been involved. The PeV neutrino event number can be $\sim 4\times 10^{-3}$ for a hard proton index $\Gamma =1.5$.

arXiv comment8 pages, MNRAS in press

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Cited by in corpus (11)

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• Interpretation of the observed neutrino emission from three Tidal Disruption Events
• Jet-cloud/star interaction as an interpretation of neutrino outburst from the blazar TXS 0506+056
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