Neutrino Emission from an Off-Axis Jet Driven by the Tidal Disruption Event AT2019dsg
Ruo-Yu Liu, Shao-Qiang Xi, Xiang-Yu Wang

TL;DR
This paper proposes that neutrino emissions from TDE AT2019dsg can be explained by off-axis jet interactions, with high opacity obscuring cascade emissions, suggesting many TDEs may produce neutrinos without detectable X-ray or gamma-ray counterparts.
Contribution
It introduces a model where off-axis jets in TDEs produce neutrinos through hadronic interactions, accounting for observed neutrino events without strong X-ray or gamma-ray signals.
Findings
Neutrino emission can originate from off-axis TDE jets.
High gas column density obscures cascade emissions in X-ray and GeV bands.
Off-axis TDE jets are more common, increasing the likelihood of neutrino detection.
Abstract
Recently, a high-energy muon neutrino event was detected in association with a tidal disruption event (TDE) AT2019dsg at the time about 150 days after the peak of the optical/UV luminosity. We propose that such a association could be interpreted as arising from hadronic interactions between relativistic protons accelerated in the jet launched from the TDE and the intense radiation field of TDE inside the optical/UV photosphere, if we are observing the jet at a moderate angle (i.e., approximately 10-30 degree) with respect to the jet axis. Such an off-axis viewing angle leads to a high gas column density in the line of sight which provides a high opacity for the photoionization and the Bethe-Heitler process, {and allows the existence of an intrinsic long-term X-ray radiation of comparatively high emissivity}. As a result, the cascade emission accompanying the neutrino production, which…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
