A commend on "Three Classes of Newtonian Three-Body Planar Periodic Orbits" by Šuvakov and Dmitrašinović (PRL, 2013)
arXiv:1312.6796 · doi:10.1007/s11433-014-5563-5
Abstract
Currently, the fifteen new periodic solutions of Newtonian three-body problem with equal mass were reported by Šuvakov and Dmitrašinović (PRL, 2013) [1]. However, using a reliable numerical approach (namely the Clean Numerical Simulation, CNS) that is based on the arbitrary-order Taylor series method and data in arbitrary-digit precision, it is found that at least seven of them greatly depart from the periodic orbits after a long enough interval of time. Therefore, the reported initial conditions of at least seven of the fifteen orbits reported by Šuvakov and Dmitrašinović [1] are not accurate enough to predict periodic orbits. Besides, it is found that these seven orbits are unstable.
5 pages, 5 figures
References in corpus (1)
Cited by in corpus (7)
- More than six hundreds new families of Newtonian periodic planar collisionless three-body orbits
- Ultra-chaos: an insurmountable objective obstacle of reproducibility and replicability
- On the origin of intrinsic randomness of Rayleigh-Benard turbulence
- On the inherent self-excited macroscopic randomness of chaotic three-body system
- One family of 13315 stable periodic orbits of the non-hierarchical unequal-mass triple system
- The influence of numerical noises on statistics computation of chaotic dynamic systems
- Clean Numerical Simulation: A New Strategy to Obtain Reliable Solutions of Chaotic Dynamic Systems