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...
Autors principals: | Boekholt, TCN, Portegies Zwart, SF, Valtonen, M |
---|---|
Format: | Journal article |
Idioma: | English |
Publicat: |
Oxford University Press
2020
|
Ítems similars
-
Numerical verification of the microscopic time reversibility of Newton’s equations of motion: fighting exponential divergence
per: Portegies Zwart, SF, et al.
Publicat: (2018) -
The origin of chaos in the orbit of comet 1P/Halley
per: Boekholt, TCN, et al.
Publicat: (2016) -
Relativistic Pythagorean three-body problem
per: Boekholt, TCN, et al.
Publicat: (2021) -
Chaos in self-gravitating many-body systems Lyapunov time dependence of N and the influence of general relativity
per: Zwart, SFP, et al.
Publicat: (2022) -
A direct N-body integrator for modelling the chaotic, tidal dynamics of multibody extrasolar systems: TIDYMESS
per: Boekholt, TCN, et al.
Publicat: (2023)