Internal Dynamics of Neutron Stars
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چکیده
Internal Dvnamics of Neutron Stars The central element of many binary x-ray sources is a neutron star. Advances in the theory of dense matter, spurred by precise measurements of changes in spin rates of both rotationpowered and accretion-powered pulsars (see, for example, the section entitled “High-Mass X-Ray Binaries” in the main text) has made it possible to build detailed models describing the properties of these stars. The latest work has led to a dramatic reversal of earlier views.
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