The nonradial oscillation spectra of neutron stars

Details The nonradial oscillation spectra of neutron stars The nonradial oscillation spectra of neutron stars

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...297l..37m&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 297, Oct. 15, 1985, p. L37-L40.

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Neutron Stars, Pulsars, Stellar Oscillations, Stellar Spectra, Vibration Mode, Computational Astrophysics, Stellar Structure

Scientific paper

The authors have computed nonradial oscillation spectra for a number of realistic, finite-temperature, nonrotating, nonmagnetic neutron stars containing solid crusts. The spectra consist of p-modes (with periods Π < 0.2 ms), g-modes trapped in the fluid "ocean" layer (Π > 100 ms), g-modes trapped in the fluid core (Π > 10 s), shear (s-) and toroidal (t-) modes confined to the solid crust (Π < 1 ms), and interfacial (i-) modes associated with the stellar surface (f-mode: Π ≈ 0.2 - 0.4 ms), the "ocean"/crust interface (Π ≈ 10 - 100 ms), and the crust/core interface (Π ≈ 10 - 100 ms).

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