A small asymmetry in the flux of neutrinos emitted by a hot newly-born
neutron star could explain the observed motions of pulsars. However,
even in the presence of parity-violating processes with anisotropic sc
attering amplitudes, no asymmetry is generated in thermal equilibrium.
We explain why this no-go theorem stymies some of the proposed explan
ations for the pulsar ''kick'' velocities. (C) 1998 Elsevier Science B
.V. All rights reserved.