Inertial waves near corotation in three-dimensional hydrodynamical discs

被引:13
作者
Latter, Henrik N. [1 ]
Balbus, Steven A. [1 ]
机构
[1] Ecole Normale Super, Lab Radioastron, F-75005 Paris, France
关键词
accretion; accretion discs; hydrodynamics; instabilities; waves; G-MODE OSCILLATIONS; DIFFERENTIALLY ROTATING-DISKS; ANGULAR-MOMENTUM TRANSPORT; THIN RELATIVISTIC DISKS; ACCRETION DISKS; DYNAMICAL STABILITY; LINEAR-THEORY; INSTABILITY; EXCITATION; FLOW;
D O I
10.1111/j.1365-2966.2009.15350.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:1058 / 1073
页数:16
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