Acta mathematica scientia,Series B ›› 2015, Vol. 35 ›› Issue (6): 1359-1385.doi: 10.1016/S0252-9602(15)30060-6

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RAYLEIGH-TAYLOR INSTABILITY FOR COMPRESSIBLE ROTATING FLOWS

Ran DUAN1, Fei JIANG2, Fei JIANG3   

  1. 1. School of Mathematics and Statistics, Central China Normal University, Wuhan 430079, China;
    2. College of Mathematics and Computer Science, Fuzhou University, Fuzhou 361000, China;
    3. Institute of Applied Physics and Computational Mathematics, Beijing 100088, China
  • Received:2015-02-15 Revised:2014-08-26 Online:2015-11-01 Published:2015-11-01
  • Supported by:

    The research of Ran Duan was supported by three grants from the NSFC (11001096, 11471134), Program for Changjiang Scholars and Innovative Research Team in University (IRT13066); the research of Fei Jiang and Junping Yin was supported by NSFC (11101044, 11301083).

Abstract:

In this paper, we investigate the Rayleigh-Taylor instability problem for two compressible, immiscible, inviscid flows rotating with a constant angular velocity, and evolving with a free interface in the presence of a uniform gravitational field. First we construct the Rayleigh-Taylor steady-state solutions with a denser fluid lying above the free interface with the second fluid, then we turn to an analysis of the equations obtained from linearization around such a steady state. In the presence of uniform rotation, there is no natural variational framework for constructing growing mode solutions to the linearized problem. Using the general method of studying a family of modified variational problems introduced in etc|ξ|-1,where ξ is the spatial frequency of the normal mode and the constant c depends on some physical parameters of the two layer fluids. A Fourier synthesis of these normal mode solutions allows us to construct solutions that grow arbitrarily quickly in the Sobolev space Hk, and leads to an ill-posedness result for the linearized problem. Moreover, from the analysis we see that rotation diminishes the growth of instability. Using the pathological solutions, we then demonstrate the ill-posedness for the original non-linear problem in some sense.

Key words: Rayleigh-Taylor instability, rotation, Hadamard sense

CLC Number: 

  • 35L65
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