Computer Science
Scientific paper
Oct 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993hadj...16..349b&link_type=abstract
Hadronic J., Vol. 16, No. 5, p. 349 - 355
Computer Science
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.
Bastrukov S. I.
Piliugin E. N.
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