SN 2023uqf, a rare interacting Type Ibn supernova found coincident with neutrino IC231004A, is the first observational evidence that interacting supernovae are hadronic accelerators.
Search for Neutrinos from Populations of Optical Transients
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abstract
Since the detection of high-energy cosmic neutrinos at the IceCube Neutrino Observatory in 2013, there has been an on-going search to find the origins of this flux. Despite recent evidence identifying a flaring blazar as a possible neutrino source, the vast majority of the diffuse neutrino flux measured by IceCube remains unexplained. Here, the latest IceCube results testing time-dependent correlation between neutrinos and Tidal Disruption Events (TDEs) are presented, limiting the contribution of jetted and non-jetted TDEs to the diffuse astrophysical neutrino flux to be less than 1.3% and 26% respectively at 90% confidence level. In addition, a dedicated search for neutrinos from the extraordinary transient AT2018cow are presented, and upper limits on the integrated neutrino emission are derived. Expected improvements from new and upcoming time domain optical surveys (such as ZTF and LSST) are also introduced.
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SN 2023uqf: An Interacting Supernova Coincident with a High-Energy Neutrino
SN 2023uqf, a rare interacting Type Ibn supernova found coincident with neutrino IC231004A, is the first observational evidence that interacting supernovae are hadronic accelerators.