Crustal Oscillations of Slowly Rotating Relativistic Stars

Abstract

We study low-amplitude crustal oscillations of slowly rotating relativistic stars consisting of a central fluid core and an outer thin solid crust. We estimate the effect of rotation on the torsional toroidal modes and on the interfacial and shear spheroidal modes. The results compared against the Newtonian ones for wide range of neutron star models and equations of state.

15 pages

References in corpus (9)

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Cited by in corpus (12)

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• Stellar Oscillations in Tensor-Vector-Scalar Theory
• General-relativistic treatment of tidal $g$-mode resonances in coalescing binaries of neutron stars. I. Theoretical framework and crust breaking
• Dynamics of Fast Rotating Neutron Stars: An Approach in the Hilbert Gauge
• Fast Rotating Neutron Stars: Oscillations and Instabilities
• Slowly Rotating Relativistic Stars in Tensor-Vector-Scalar Theory
• Measuring spin in coalescing binaries of neutron stars showing double precursors
• Impact of the relativistic Cowling approximation on shear and interface modes of neutron stars