Stationary structure of relativistic superfluid neutron stars

Simple item page
dc.creatorPrix, R.
dc.creatorNovak, J.
dc.creatorComer, G. L.
dc.date2002-11-29
dc.date.accessioned2026-07-07T03:27:21Z
dc.date.available2026-07-07T03:27:21Z
dc.descriptionWe describe recent progress in the numerical study of the structure of rapidly rotating superfluid neutron star models in full general relativity. The superfluid neutron star is described by a model of two interpenetrating and interacting fluids, one representing the superfluid neutrons and the second consisting of the remaining charged particles (protons, electrons, muons). We consider general stationary configurations where the two fluids can have different rotation rates around a common rotation axis. The previously discovered existence of configurations with one fluid in a prolate shape is confirmed.
dc.description5 pages, 2 figures. Conference proceedings for the 26th Spanish Relativity Meeting (ERE 2002), Menorca, Spain, 22-24 Sept. 2002
dc.identifierhttps://arxiv.org/abs/gr-qc/0211105
dc.identifierhttp://arxiv.org/abs/gr-qc/0211105
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34402
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleStationary structure of relativistic superfluid neutron stars
dc.typetext

Files

Collections

arXiv