Global chaoticity in the Pythagorean three-body problem |
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| Authors: | S J Aarseth J P Anosova V V Orlov V G Szebehely |
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| Institution: | (1) Institute of Astronomy, University of Cambridge, Madingley Road, CB3 0HA Cambridge, England;(2) Astronomical Observatory, St. Petersburg University, Bibliotechnaya pl. 2, 198904 St. Petersburg, Petrodvorets, Russia;(3) Department of Aerospace Engineering and Engineering Mechanics, University of Texas at Austin, 78712-1085 Austin, Texas, U.S.A. |
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| Abstract: | The effects of small changes in the initial conditions of the Pythagorean three-body problem are investigated by computer simulations. This problem consists of three interacting bodies with masses 3, 4 and 5 placed with zero velocities at the apices of a triangle with sides 3, 4 and 5. The final outcome of this motion is that two bodies form a binary and the third body escapes. We attempt to establish regions of the initial positions which give regular and chaotic motions. The vicinity of a small neighbourhood around the standard initial position of each body defines a regular region. Other regular regions also exist. Inside these regions the parameters of the triple systems describing the final outcome change continuously with the initial positions. Outside the regular regions the variations of the parameters are abrupt when the initial conditions change smoothly. Escape takes place after a close triple approach which is very sensitive to the initial conditions. Time-reversed solutions are employed to ensure reliable numerical results and distinguish between predictable and non-predictable motions. Close triple approaches often result in non-predictability, even when using regularization; this introduces fundamental difficulties in establishing chaotic regions. |
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| Keywords: | Three-body problem chaotic motions regularization |
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