Perturbed phase-space dynamics of hard-disk fluids

被引:40
作者
Forster, C
Hirschl, R
Posch, HA
Hoover, WG
机构
[1] Univ Vienna, Inst Expt Phys, A-1090 Vienna, Austria
[2] Univ Vienna, Inst Mat Phys, A-1090 Vienna, Austria
[3] Univ Calif Davis, Dept Appl Sci, Livermore, CA 94551 USA
[4] Lawrence Livermore Natl Lab, Methods Dev Grp, Livermore, CA 94551 USA
关键词
hydrodynamic modes; lyapunov spectrum; localized modes; fluid dynamics;
D O I
10.1016/j.physd.2003.09.013
中图分类号
O29 [应用数学];
学科分类号
070104 ;
摘要
The Lyapunov spectrum describes the exponential growth, or decay, of infinitesimal phase-space perturbations. The perturbation associated with the maximum Lyapunov exponent is strongly localized in space, and only a small fraction of all particles contributes to the perturbation growth at any instant of time. This fraction converges to zero in the thermodynamic large-particle-number limit. For hard-disk and hard-sphere systems the perturbations belonging to the smallest of the non-vanishing exponents are coherently spread out and form orthogonal periodic structures in space, the "Lyapunov modes". There are two types of mode polarizations, transverse and longitudinal. The transverse modes do not propagate, but the longitudinal modes do, with a speed about one third of the sound speed. We characterize the symmetry and the degeneracy of the modes. In the thermodynamic limit the Lyapunov spectrum has a diverging slope near the intersection with the abscissa. No positive lower bound exists for the positive exponents. The mode amplitude scales with the inverse square root of the particle number as expected from the normalization of the perturbation vectors. (C) 2003 Elsevier B.V. All rights reserved.
引用
收藏
页码:294 / 310
页数:17
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