作者: J. A. Sauls , D. L. Stein , J. W. Serene
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摘要: /sup 3/P/sub 2/ vortices in neutron-star matter are structurally different from a 1/S/sub 0/ superfluid. The most important difference is that have spontaneous magnetization the core region directed along vortex line. We estimate velocity relaxation time for electron scattering these and compare our results with those of Feibelman observed times Crab Vela pulsars.