Computer Science – Sound
Scientific paper
Oct 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...333..880e&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 333, Oct. 15, 1988, p. 880-894. DOE-sponsored research.
Computer Science
Sound
48
Acoustic Properties, Neutron Stars, Stellar Structure, Wave Propagation, Acoustic Velocity, Propagation Modes, Stellar Cores, Superfluidity, Velocity Distribution
Scientific paper
Neutron and proton superfluidity alters sound wave propagation in the interior of a neutron star. The partial decoupling of the motions of different components of the matter creates new modes and modifies the previously known modes. This paper presents the sound velocities and the relative displacements of the different components for short-wavelength longitudinal and transverse oscillations in neutron star matter. The new compressional and shear modes that a neutron star can support are discussed.
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