Linear coupling of modes in two-dimensional radially stratified astrophysical discs

被引:12
作者
Tevzadze, A. G. [1 ]
Chagelishvili, G. D. [1 ,2 ]
Bodo, G. [3 ]
Rossi, P. [3 ]
机构
[1] Chavchavadze State Univ, Georgian Natl Astrophys Observ, Tbilisi, Georgia
[2] Georgian Acad Sci, Nodia Inst Geophys, GE-380060 Tbilisi, Georgia
[3] Osserv Astron Torino, INAF, I-10025 Pino Torinese, Italy
关键词
accretion; accretion discs; hydrodynamics; instabilities; BAROCLINIC VORTICITY PRODUCTION; ROSSBY-WAVE INSTABILITY; SPIRAL DENSITY WAVES; PROTOPLANETARY DISKS; ACCRETION DISKS; TURBULENT FLUCTUATIONS; HYDRODYNAMIC STABILITY; TRANSIENT GROWTH; VORTEX; THIN;
D O I
10.1111/j.1365-2966.2009.15723.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigate mode coupling in a two-dimensional compressible disc with radial stratification and differential rotation. We employ the global radial scaling of linear perturbations and study the linear modes in the local shearing-sheet approximation. We employ a three-mode formalism and study the vorticity (W), entropy (S) and compressional (P) modes and their coupling properties. The system exhibits asymmetric three-mode coupling: this includes mutual coupling of S and P modes, S and W modes, and asymmetric coupling between the W and P modes. P-mode perturbations are able to generate potential vorticity through indirect three-mode coupling. This process indicates that compressional perturbations can lead to the development of vortical structures and influence the dynamics of radially stratified hydrodynamic accretion and protoplanetary discs.
引用
收藏
页码:901 / 912
页数:12
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