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.
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Submitted on 22 Mar 2001 (v1), last revised 23 Apr 2001 (this version, v7)
Updated
arXiv.org
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