Fundamental frequencies of elastic gravitational vibrations of a neutron star.

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Scientific paper

The long wavelength vibrations of a homogeneous non-rotating neutron star are studied within the framework of the nuclear fluid-dynamics. The stellar continuum is modelled by incompressible hadronic matter with properties of an isotropic elastic solid. The equilibrium and large-scale dynamics of the neutron star is presumed to be dominated by Newtonian self-gravtiy. The eigenfrequencies of spheroidal and torsional elastic-gravitational vibrations are derived in analytic form.

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