Dark matter seeding and the kinematics and rotation of neutron stars
  Self-annihilation of dark matter accreted from the galactic halo in the inner
regions of neutron stars may affect their kinematical properties, namely
velocity kicks and rotation patterns. We find that if a stable long-lived
single or multiple strangelet off-center seed forms, there is an associated
change in momentum and torque that may affect the kinematical observables of
the star.
