Chaos in self-gravitating many-body systems Lyapunov time dependence of N and the influence of general relativity
In self-gravitating N-body systems, small perturbations introduced at the start, or infinitesimal errors that are produced by the numerical integrator or are due to limited precision in the computer, grow exponentially with time. For Newton's gravity, we confirm earlier results that for relativ...
Autori principali: | Zwart, SFP, Boekholt, TCN, Por, EH, Hamers, AS, McMillan, SLW |
---|---|
Natura: | Journal article |
Lingua: | English |
Pubblicazione: |
EDP Sciences
2022
|
Documenti analoghi
-
Relativistic Pythagorean three-body problem
di: Boekholt, TCN, et al.
Pubblicazione: (2021) -
Gargantuan chaotic gravitational three-body systems and their irreversibility to the Planck length
di: Boekholt, TCN, et al.
Pubblicazione: (2020) -
Velocity-dependent Lyapunov exponents in many-body quantum, semiclassical, and classical chaos
di: Khemani, V, et al.
Pubblicazione: (2018) -
The origin of chaos in the orbit of comet 1P/Halley
di: Boekholt, TCN, et al.
Pubblicazione: (2016) -
Stellar triples on the edge: Comprehensive overview of the evolution of destabilised triples leading to stellar and binary exotica
di: Toonen, S, et al.
Pubblicazione: (2022)