Inertial waves near corotation in three-dimensional hydrodynamical discs

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Abstract

This paper concerns the interaction between non-axisymmetric inertial waves and their corotation resonances in a hydrodynamical disc. Inertial waves are of interest because they can localize in resonant cavities circumscribed by Lindblad radii and, as a consequence, can exhibit discrete oscillation frequencies that may be observed. It is often hypothesized that these trapped eigenmodes are affiliated with the poorly understood quasi-periodic oscillation phenomenon. We demonstrate that a large class of non-axisymmetric three-dimensional (3D) inertial waves cannot manifest as trapped normal modes. This class includes any inertial wave whose resonant cavity contains a corotation singularity. Instead, these 'singular' modes constitute a continuous spectrum and, as an ensemble, are convected with the flow, giving rise to shearing waves. Finally, we present a simple demonstration of how the corotation singularity stabilizes 3D perturbations in a slender torus. © 2009 RAS.

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Latter, H. N., & Balbus, S. A. (2009). Inertial waves near corotation in three-dimensional hydrodynamical discs. Monthly Notices of the Royal Astronomical Society, 399(2), 1058–1073. https://doi.org/10.1111/j.1365-2966.2009.15350.x

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