General-Relativistic Curvature of Pulsar Vortex Structure
arXiv:astro-ph/0103366 · doi:10.1134/1.1368700
Abstract
The motion of a neutron superfluid condensate in a pulsar is studied. Several theorems of general-relativistic hydrodynamics are proved for a superfluid. The average density distribution of vortex lines in pulsars and their general-relativistic curvature are derived.
18 pages, 1 figures