Jet-induced explosions of core collapse supernovae

We numerically studied the explosion of a supernova caused by supersonic je ts present in its center. The jets are assumed to be generated by a magneto rotational mechanism when a stellar core collapses into a neutron star. We simulated the process of the jet propagation through the star, jet breakthr ough, and the ejection of the supernova envelope by the lateral shocks gene rated during jet propagation. The end result of the interaction is a highly nonspherical supernova explosion with two high-velocity jets of material m oving in polar directions and slower moving, oblate, highly distorted eject a containing most of the supernova material. The jet-induced explosion is e ntirely due to the action of the jets on the surrounding star and does not depend on neutrino transport or reacceleration of a stalled shock. The jet mechanism can explain the observed high polarization of Types Ib, Ic, and I Isupernovae, pulsar kicks, very high velocity material observed in supernov a remnants, indications that radioactive material was carried to the hydrog en-rich layers in SN 1987A, and other observations that are very difficult or impossible to explain by the neutrino energy deposition mechanism. The b reakout of the jet from a compact, hydrogen-deficient core may account for the gamma-ray burst and radio outburst associated with SN 1998bw/ GRB 98042 5.