Dynamical Instability of Laminar Axisymmetric Flow of Perfect Fluid with Stratification

Details Dynamical Instability of Laminar Axisymmetric Flow of Perfect Fluid with Stratification Dynamical Instability of Laminar Axisymmetric Flow of Perfect Fluid with Stratification

2007-09-12

arxiv.org/abs/0709.1833v1

Astronomy and Astrophysics

Astrophysics

19 pages, 7 figures, accepted to AstL

Scientific paper

10.1134/S1063773707110059

The instability of non-homoentropic axisymmetric flow of perfect fluid with respect to non-axisymmetric infinitesimal perturbations was investigated by numerical integration of hydrodynamical differential equations in two-dimensional approximation. The non-trivial influence of entropy gradient on unstable sound and surface gravity waves was revealed. In particular, both decrease and growth of entropy against the direction of effective gravitational acceleration $g_{eff}$ give rise to growing surface gravity modes which are stable with the same parameters in the case of homoentropic flow. At the same time increment of sound modes either grows monotonically while the rate of entropy decrease against $g_{eff}$ gets higher or vanishes at some values of positive and negative entropy gradient in the basic flow. The calculations have showed also that growing internal gravity modes appear only in the flow unstable to axisymmetric perturbations. At last, the analysis of boundary problem with free boundaries uncovered that's incorrect to set the entropy distribution according to polytropic law with polytropic index different from adiabatic value, since in this case perturbations don't satisfy the free boundary conditions.

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