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Supernova (SN) 2023ixf in M101 is the closest SN explosion observed in thelast decade. Therefore it is a suitable test bed to study the role of jets inpowering the SN ejecta. With this aim, we explored the idea that high-energyneutrinos could be produced during the interaction between the jets and theintense radiation field produced in the SN explosion and eventually be observedby the IceCube neutrino telescope. The lack of detection of such neutrinos hassignificantly constrained both the fraction of stellar collapses that producejets and/or the theoretical models for neutrino production. Finally, weinvestigated the possibility of detecting low-energy neutrinos from SN 2023ixfwith the Super- and Hyper-Kamiokande experiments, obtaining in both casessub-threshold estimates.

Low and High Energy Neutrinos from SN 2023ixf in M101