  Supernova (SN) 2023ixf in M101 is the closest SN explosion observed in the
last decade. Therefore it is a suitable test bed to study the role of jets in
powering the SN ejecta. With this aim, we explored the idea that high-energy
neutrinos could be produced during the interaction between the jets and the
intense radiation field produced in the SN explosion and eventually be observed
by the IceCube neutrino telescope. The lack of detection of such neutrinos has
significantly constrained both the fraction of stellar collapses that produce
jets and/or the theoretical models for neutrino production. Finally, we
investigated the possibility of detecting low-energy neutrinos from SN 2023ixf
with the Super- and Hyper-Kamiokande experiments, obtaining in both cases
sub-threshold estimates.
