Rotation of a two-component model neutron star in the GTR.

Details Rotation of a two-component model neutron star in the GTR. Rotation of a two-component model neutron star in the GTR.

Jul 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ap.....40..260s&link_type=abstract

Astrophysics, Volume 40, Issue 3, pp.260-266

Astronomy and Astrophysics

Astrophysics

1

Neutron Stars: General Relativity

Scientific paper

Equations are obtained for the dynamics of the rotation of a two-component model neutron star within the framework of the generai theory of relativity. It is shown that for steady rotation of the star’s normal component, Ωc = const, the angular velocity Ωs of the superfluid component depends on the coordinates and is Ωc + ω, where ω is the nondiagonal component of the metric tensor.

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