Mapping the three-body system -: decay time and reversibility

被引:5
作者
Lehto, H. J. [1 ,2 ]
Kotiranta, S. [1 ,2 ]
Valtonen, M. J. [1 ,2 ]
Heinamaki, P. [1 ,2 ]
Mikkola, S. [1 ,2 ]
Chernin, A. D. [1 ,2 ,3 ]
机构
[1] Univ Turku, Dept Phys, FI-21500 Piikkio, Finland
[2] Univ Turku, Tuorla Observ, FI-21500 Piikkio, Finland
[3] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow, Russia
关键词
methods : N-body simulations; celestial mechanics;
D O I
10.1111/j.1365-2966.2008.13450.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Ill this paper we carry out a quantitative analysis of the three-body systems and map them as a function of decaying time and initial configuration, look at this problem as ail example of a simple deterministic system and ask to what extent the orbits are really predictable. We have investigated the behaviour of about 200000 general Newtonian three-body systems using the simplest initial conditions. Within Our resolution these cover all file possible states where the objects are initially at rest and have no angular momentum. We have determined the decay time-scales of the triple systems and show that the distribution of this parameter is fractal in appearance. Some areas that appear stable on large scales exhibit very narrow strips of instability and the overall pattern, dominated by resonances, reminds us of a traditional Maasai warrior shield. Also an attempt is made to recover the original starting configuration of the three bodies by backward integration. We find there are instances where the evolution to the future and to the past lead to different orbits, in spite of time symmetric initial conditions. This implies that even in simple deterministic systems there exists an arrow of time.
引用
收藏
页码:965 / 970
页数:6
相关论文
共 26 条
[1]   GLOBAL CHAOTICITY IN THE PYTHAGOREAN 3-BODY PROBLEM [J].
AARSETH, SJ ;
ANOSOVA, JP ;
ORLOV, VV ;
SZEBEHELY, VG .
CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY, 1994, 58 (01) :1-16
[2]  
Agekyan T.A., 1967, Soviet Phys. Astron., V44, P1261
[3]  
[Anonymous], 1984, ORDER OUT CHAOS
[4]   DYNAMIC EVOLUTION OF TRIPLE-SYSTEMS [J].
ANOSOVA, JP .
ASTROPHYSICS AND SPACE SCIENCE, 1986, 124 (02) :217-241
[5]   Time evolution of thermodynamic entropy for conservative and dissipative chaotic maps [J].
Baranger, M ;
Latora, V ;
Rapisarda, A .
CHAOS SOLITONS & FRACTALS, 2002, 13 (03) :471-478
[6]   FROM INSTABILITY TO IRREVERSIBILITY [J].
ELSKENS, Y ;
PRIGOGINE, I .
PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA, 1986, 83 (16) :5756-5760
[7]  
Hausdorff F, 1919, MATH ANN, V79, P157
[8]   BINARY EVOLUTION IN STELLAR DYNAMICS [J].
HEGGIE, DC .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1975, 173 (03) :729-787
[9]   Chaos in three-body dynamics:: Kolmogorov-Sinai entropy [J].
Heinämäki, P ;
Lehto, HJ ;
Valtonen, MJ ;
Chernin, AD .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1999, 310 (03) :811-822
[10]  
Huntingford G. W. B., 1961, J ROYAL ANTHR I GREA, V91, P251, DOI DOI 10.2307/2844416