Velocity-dependent energy gaps and dynamics of superfluid neutron stars
  We show that suppression of the baryon energy gaps, caused by the relative motion of superfluid and normal liquid components, can substantially influence dynamical properties and evolution of neutron stars. This effect has been previously ignored in the neutron-star literature. 
M. E. Gusakov, E. M. Kantor (Ioffe Institute)
astro-ph.SR astro-ph.HE nucl-th