COMMENTS ON THE COMPUTATION OF LIAPUNOV EXPONENTS FOR THE MIXMASTER UNIVERSE

被引:42
作者
BERGER, BK
机构
[1] Physics Department, Oakland University, Rochester, 48309, Michigan
关键词
D O I
10.1007/BF00756831
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
To explain the discrepancy between recently computed vanishing Liapunov exponents for the evolution of Mixmaster universes and the positive Liapunov exponent for the associated 1-dimensional map first discussed by Belinskii, Khalatnikov, and Lifshitz, the Liapunov exponents computed from a numerical universe evolution are compared using several time variables. Previous numerical results of vanishing Liapunov exponents were obtained with time variables which increased roughly exponentially in each epoch. Here it is found that minisuperspace proper time, which increases by a fixed amount during each epoch, yields non-vanishing Liapunov exponents within the limited number of epochs numerically accessible. The map parameter u as measured along the trajectory attains the values predicted by the map to very high accuracy (except near the maximum of expansion) even though the metric coefficients deviate in some cases from idealized Mixmaster behavior. The number of consecutive single epoch eras is shown to be related to the presence of u in an interval bounded by ratios of Fibonacci numbers.
引用
收藏
页码:1385 / 1402
页数:18
相关论文
共 33 条
[31]   A DYNAMICAL-SYSTEMS APPROACH TO BIANCHI COSMOLOGIES - ORTHOGONAL MODELS OF CLASS-A [J].
WAINWRIGHT, J ;
HSU, L .
CLASSICAL AND QUANTUM GRAVITY, 1989, 6 (10) :1409-1431
[32]   DETERMINING LYAPUNOV EXPONENTS FROM A TIME-SERIES [J].
WOLF, A ;
SWIFT, JB ;
SWINNEY, HL ;
VASTANO, JA .
PHYSICA D, 1985, 16 (03) :285-317
[33]  
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