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Since the detection of high-energy cosmic neutrinos at the IceCube NeutrinoObservatory in 2013, there has been an on-going search to find the origins ofthis flux. Despite recent evidence identifying a flaring blazar as a possibleneutrino source, the vast majority of the diffuse neutrino flux measured byIceCube remains unexplained. Here, the latest IceCube results testingtime-dependent correlation between neutrinos and Tidal Disruption Events (TDEs)are presented, limiting the contribution of jetted and non-jetted TDEs to thediffuse astrophysical neutrino flux to be less than 1.3% and 26% respectivelyat 90% confidence level. In addition, a dedicated search for neutrinos from theextraordinary transient AT2018cow are presented, and upper limits on theintegrated neutrino emission are derived. Expected improvements from new andupcoming time domain optical surveys (such as ZTF and LSST) are alsointroduced.

Search for Neutrinos from Populations of Optical Transients