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We investigate the instability and stability of some steady-states of a three-dimensional nonhomogeneous incompressible viscous flow driven by gravity in a bounded domain Omega of class C-2. When the steady density is heavier with increasing height (i.e., the Rayleigh-Taylor steady-state), we show that the steady-state is linear unstable (i.e., the linear solution grows in time in H-2) by constructing a (standard) energy functional and exploiting the modified variational method. Then, by introducing a new energy functional and using a careful bootstrap argument, we further show that the steady-state is nonlinear unstable in the sense of Hadamard. When the steady density is lighter with increasing height, we show, with the help of a restricted condition imposed on steady density, that the steady-state is linearly globally stable and nonlinearly asymptotically stable in the sense of Hadamard. (C) 2014 Elsevier Inc. All rights reserved.
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ADVANCES IN MATHEMATICS
ISSN: 0001-8708
Year: 2014
Volume: 264
Page: 831-863
1 . 2 9 4
JCR@2014
1 . 5 0 0
JCR@2023
ESI Discipline: MATHEMATICS;
ESI HC Threshold:86
JCR Journal Grade:1
CAS Journal Grade:2
Cited Count:
WoS CC Cited Count: 57
SCOPUS Cited Count: 55
ESI Highly Cited Papers on the List: 0 Unfold All
WanFang Cited Count:
Chinese Cited Count:
30 Days PV: 2
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