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The era of multimessenger astrophysics with high-energy neutrinos began with the discovery of high-energy astrophysical neutrinos in IceCube in 2013. Today, after a decade of observation, sign of anisotropy has emerged in the arrival direction of cosmic neutrinos. IceCube has identified neutrino emission from a nearby active galaxies and uncovered a subdominant neutrino emission from the Milky Way. In this talk, I will review these recent results and will discuss the emerging multimessenger picture for the origin of high-energy neutrinos and the new opportunities they offer to search for physics beyond the Standard Model in the neutrino sector.
https://bnl.zoomgov.com/j/1653048131?pwd=fkT0TgSQn5wqXX55rQa3jABDwMj8sE.1