  A fraction of core collapse supernovae of type Ib/c are associated with
Gamma-ray bursts, which are thought to produce highly relativistic jets.
Recently, it has been hypothesized that a larger fraction of core collapse
supernovae produce slower jets, which may contribute to the disruption and
ejection of the supernova envelope, and explain the unusually energetic
hypernovae. We explore the TeV neutrino signatures expected from such slower
jets, and calculate the expected detection rates with upcoming Gigaton
Cherenkov experiments. We conclude that individual jetted SNe may be detectable
from nearby galaxies.
