Effect of background magnetic field on the normal modes of conformal
  dissipative chiral hydro and a novel mechanism for explaining pulsar kicks
  In the present work, we have studied the collective behaviour of a chiral
plasma with first and second order dissipative corrections allowed by conformal
symmetry. We have derived dispersion relations for ideal, first order and
second order MHD for the chiral plasma. We have also used our results to
explain the observed pulsar kicks.
