On the timescales in the chaotic dynamics of a 4D symplectic map

被引:0
作者
Cincotta, Pablo M. [1 ,2 ]
Giordano, Claudia M. [1 ,2 ]
机构
[1] Univ Nacl La Plata, Fac Ciencias Astron & Geofis, Grp Caos Sistemas Hamiltonianos, Paseo Bosque S-N,B1900FWA, La Plata, Argentina
[2] Inst Astrofis La Plata CONICET, Paseo Bosque S-N,B1900FWA, La Plata, Argentina
关键词
ARNOLD DIFFUSION; GLOBAL DYNAMICS; INSTABILITY; SYSTEMS; TRANSPORT;
D O I
10.1063/5.0232321
中图分类号
O29 [应用数学];
学科分类号
070104 ;
摘要
In this work, we investigate different timescales of chaotic dynamics in a multi-parametric 4D symplectic map. We compute the Lyapunov time and a macroscopic timescale, the instability time, for a wide range of values of the system's parameters and many different ensembles of initial conditions in resonant domains. The instability time is obtained by plain numerical simulations and by its estimates from the diffusion time, which we derive in three different ways: through a normal and an anomalous diffusion law and by the Shannon entropy, whose formulation is briefly revisited. A discussion about which of the four approaches provide reliable values of the timescale for a macroscopic instability is addressed. The relationship between the Lyapunov time and the instability time is revisited and studied for this particular system where in some cases, an exponential or polynomial law has been observed. The main conclusion of the present research is that only when the dynamical system behaves as a nearly ergodic one such relationship arises and the Lyapunov and instability times are global timescales, independent of the position in phase space. When stability regions prevent the free diffusion, no correlations between both timescales are observed, they are local and depend on both the position in phase space and the perturbation strength. In any case, the instability time largely exceeds the Lyapunov time. Thus, when the system is far from nearly ergodic, the timescale for predictable dynamics is given by the instability time, being the Lyapunov time its lower bound.
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页数:17
相关论文
共 52 条
[1]   Instability times in the HD 181433 exoplanetary system [J].
Alves Silva, R. ;
Beauge, C. ;
Ferraz-Mello, S. ;
Cincotta, P. M. ;
Giordano, C. M. .
ASTRONOMY & ASTROPHYSICS, 2021, 652
[2]  
Arnold V., 1989, ERGODIC PROBLEMS CLA
[3]  
ARNOLD VI, 1964, DOKL AKAD NAUK SSSR+, V156, P9
[4]  
Benettin G, 1980, MECCANICA, V15, P21, DOI [10.1007/BF02128237, DOI 10.1007/BF02128237]
[5]  
Chirikov B. V., 1996, Journal of Experimental and Theoretical Physics, V83, P646
[6]   UNIVERSAL INSTABILITY OF MANY-DIMENSIONAL OSCILLATOR SYSTEMS [J].
CHIRIKOV, BV .
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 1979, 52 (05) :263-379
[7]   Estimation of the diffusion time in a triaxial galactic potential [J].
Cincotta, P. M. ;
Giordano, C. M. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023, 526 (01) :895-902
[8]   Correlations in area preserving maps: A Shannon entropy approach [J].
Cincotta, P. M. ;
Shevchenko, I. I. .
PHYSICA D-NONLINEAR PHENOMENA, 2020, 402
[9]   On the chaotic diffusion in multidimensional Hamiltonian systems [J].
Cincotta, P. M. ;
Giordano, C. M. ;
Marti, J. G. ;
Beauge, C. .
CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY, 2018, 130 (01)
[10]  
Cincotta P. M., Chaos Detection and Predictability, DOI [10.1007/978-3-662-48410-44, DOI 10.1007/978-3-662-48410-44]