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  Stationary structure of relativistic superfluid neutron stars

Prix, R., Novak, J., & Comer, G. L. (2002). Stationary structure of relativistic superfluid neutron stars.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-5380-5 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-5381-3
Genre: Conference Paper

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0211105v1.pdf (Preprint), 156KB
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 Creators:
Prix, Reinhard1, Author              
Novak, Jerome, Author
Comer, G. L., Author
Affiliations:
1Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, escidoc:24011              

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 Abstract: We 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.

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 Dates: 2002-11-09
 Publication Status: Published in print
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 Rev. Method: -
 Identifiers: eDoc: 379325
Other: arXiv:gr-qc/0211105v1
URI: http://arxiv.org/abs/gr-qc/0211105
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Title: 26th Spanish Relativity Meeting
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Start-/End Date: 2002 -

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