Gargantuan chaotic gravitational three-body systems and their irreversibility to the Planck length
Chaos is present in most stellar dynamical systems and manifests itself through the exponential growth of small perturbations. Exponential divergence drives time irreversibility and increases the entropy in the system. A numerical consequence is that integrations of the N-body problem unavoidably ma...
Auteurs principaux: | Boekholt, TCN, Portegies Zwart, SF, Valtonen, M |
---|---|
Format: | Journal article |
Langue: | English |
Publié: |
Oxford University Press
2020
|
Documents similaires
-
Numerical verification of the microscopic time reversibility of Newton’s equations of motion: fighting exponential divergence
par: Portegies Zwart, SF, et autres
Publié: (2018) -
The origin of chaos in the orbit of comet 1P/Halley
par: Boekholt, TCN, et autres
Publié: (2016) -
Relativistic Pythagorean three-body problem
par: Boekholt, TCN, et autres
Publié: (2021) -
Chaos in self-gravitating many-body systems Lyapunov time dependence of N and the influence of general relativity
par: Zwart, SFP, et autres
Publié: (2022) -
A direct N-body integrator for modelling the chaotic, tidal dynamics of multibody extrasolar systems: TIDYMESS
par: Boekholt, TCN, et autres
Publié: (2023)