Microscopic structure of a vortex line in superfluid neutron star matter

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dc.creatorDe Blasio, F. V.
dc.creatorElgaroy, O.
dc.date1998-08-20
dc.date.accessioned2026-07-07T12:33:19Z
dc.date.available2026-07-07T12:33:19Z
dc.descriptionThe microscopic structure of an isolated vortex line in superfluid neutron star matter is studied by solving the Bogoliubov-de Gennes equations. Our calculation, which is the starting point for a microscopic calculation of pinning forces in neutron stars, shows that the size of the vortex core varies differently with density, and is in general smaller than assumed in some earlier calculations of vortex pinning in neutron star crusts. The implications of this result are discussed
dc.description5 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/nucl-th/9808057
dc.identifierhttp://arxiv.org/abs/nucl-th/9808057
dc.identifierPhys.Rev.Lett.82:1815-1818,1999
dc.identifierdoi:10.1103/PhysRevLett.82.1815
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/217084
dc.subjectNuclear Theory
dc.subjectAstrophysics
dc.titleMicroscopic structure of a vortex line in superfluid neutron star matter
dc.typetext

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