Rotation of a two-component model neutron star in the GTR |
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| Authors: | D M Sedrakian |
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| Institution: | (1) Erevan State University, Armenia |
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| Abstract: | 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.
Translated from Astrofizika, Vol. 40, No. 3, pp. 403–412, August, 1997. |
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