Theoretical interpretation of the observed neutrino emission from Tidal Disruption Events
Walter Winter, Cecilia Lunardini
TL;DR
This paper presents a theoretical model explaining the observed neutrino emission from a Tidal Disruption Event, linking neutrino production to X-ray observations and timing, advancing understanding of TDEs as neutrino sources.
Contribution
It introduces a jet-based model connecting neutrino emission to observed X-ray signals in TDEs, explaining the timing of neutrino detection.
Findings
Neutrino emission can be explained by a jet model linked to X-ray observations.
The timing of neutrino detection aligns with the model's predictions.
Implications for future neutrino-TDE observations are discussed.
Abstract
The observation of a neutrino at IceCube in association with the Tidal Disruption Event (TDE) AT2019dsg has suggested TDEs as a new class of sources of astrophysical neutrinos. We present a model of this multi-messenger observation in a jetted concordance scenario, where the neutrino production is directly linked to the observed X-rays, and the timing of the neutrino observation (about 150 days post peak) can be naturally described. We briefly discuss the implications of our model for future neutrino-TDE associations.
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.