Core collapse supernovae are dominated by weakly interacting neutrinos
. This provides a unique opportunity for macroscopic parity violation.
We speculate that parity violation in a strong magnetic field can lea
d to an asymmetry in the explosion and a recoil of the newly formed ne
utron star. We estimate the size of this asymmetry from neutrino polar
ized-neutron elastic scattering, polarized electron capture and neutri
no-nucleus elastic scattering in a (partially) polarized electron gas.
(C) 1998 Elsevier Science B.V.