Abstract
$^{3}P_{2}$ vortices in neutron-star matter are structurally different from vortices in a $^{1}S_{0}$ superfluid. The most important difference is that $^{3}P_{2}$ vortices have a spontaneous magnetization in the core region directed along the vortex line. We estimate the velocity relaxation time for electron scattering from these vortices and compare our results with those of Feibelman and the observed relaxation times for the Crab and Vela pulsars.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
