Hopf bifurcation with cubic symmetry and instability of ABC flow

被引:19
作者
Ashwin, P
Podvigina, O
机构
[1] Univ Exeter, Sch Math Sci, Exeter EX4 4QE, Devon, England
[2] Observ Cote Azur, CNRS UMR 6529, F-06304 Nice 4, France
[3] Int Inst Earthquake Predict Theory & Math Geophys, Moscow 113556, Russia
[4] Moscow MV Lomonosov State Univ, Inst Mech, Lab Gen Aerodynam, Moscow 119899, Russia
来源
PROCEEDINGS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES | 2003年 / 459卷 / 2035期
关键词
fluid instability; Hopf bifurcation; ABC flow; symmetry;
D O I
10.1098/rspa.2002.1090
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
We examine the dynamics of generic Hopf bifurcation in a system that is symmetric under the action of the rotational symmetries of the cube. We classify the generic branches of periodic solutions at bifurcation; there are generically 27 branches corresponding to maximal symmetries, organized into five symmetry types. There are also up to 22 periodic solution branches of two other symmetry types. These results are found by examination of the normal form (with S-1 normal-form symmetry) for the bifurcation truncated at the third order. In addition to the periodic branches whose branching and stability we find, there are several branches of tori, homoclinic bifurcations and chaotic attractors in the dynamics of the third-order normal form. Since many of these features are not amenable to analysis, we give some numerical examples. On breaking the normal-form symmetry, there may be breakup of the branches of tori, but the predictions for the periodic solutions will be reliable. For the Navier-Stokes equations with a particular forcing, an ABC flow is a dynamically stable solution for small Reynolds numbers R. For the most symmetric case, A = B = C = 1, the first instability of this system is a Hopf bifurcation at R = 13.04 with rotational symmetry of the cube. We use our normal-form analysis to explain the observed behaviour of solutions at this primary instability. Numerical simulations show that there is supercritical branching to rotating waves that alternate between the three axes, which undergo secondary Hopf bifurcation to a 2-torus at approximately R = 13.09. The eight symmetrically related tori break up and then merge to form a chaotic attractor with full symmetry. We can explain all these features by use of the generic third-order normal form and S' normal-form symmetry-breaking terms.
引用
收藏
页码:1801 / 1827
页数:27
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