We study the neutrino interaction rates through charged as well as neutral
current weak interactions in hot, dense magnetized matter. At densities nea
r the neutrino sphere, matter in the presence of intense magnetic field is
polarized, and electrons and protons typically occupy the lowest Landau lev
el. The weak interaction rates in such a situation are severely modified le
ading to a sizable change in neutrino opacity and consequently on the locat
ion of the neutrino sphere which also gets distorted. This has implications
for pulsar velocity explanations. [S0556-2821(99)50108-2].