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Chaos in cosmological Hamiltonians
1Department of Astronomy, University of Florida, Gainesville 32611, USA.
Annals of the New York Academy of Sciences
|June 29, 2002
Summary
This study numerically investigates regular and chaotic behavior in time-dependent Hamiltonians. Chaotic segments show unique sub- or superexponential growth, distinguishing them from time-independent systems.
Area of Science:
- Physics
- Applied Mathematics
- Dynamical Systems
Background:
- Time-dependent Hamiltonians exhibit complex dynamics.
- Distinguishing regular from chaotic behavior is crucial for understanding dynamical systems.
Purpose of the Study:
- To numerically identify and characterize regular and chaotic behavior in specific time-dependent Hamiltonians.
- To differentiate chaotic dynamics in time-dependent potentials from those in time-independent potentials.
Main Methods:
- Numerical investigation of Hamiltonians of the form H(r, p, t) = p(2)/2 + V(r, t).
- Analysis of potential forms V = R(t)V0(r) or V = V0[R(t)r], where R(t) is a time-dependent scale factor.
- Assessment of sensitive dependence on initial conditions to distinguish regular and chaotic segments.
Main Results:
- Chaotic segments in these potentials display sub- or superexponential growth of initial perturbations, unlike time-independent potentials.
- Regular segments, though not periodic, show simpler shapes, topologies, and Fourier spectra.
- A transition between regular and chaotic behavior within a single orbit segment was observed.
Conclusions:
- The observed phenomena of regular and chaotic behavior in time-dependent Hamiltonians can be explained by a simple theoretical model.
- Sensitive dependence on initial conditions, with specific growth rates, serves as a key differentiator for chaotic behavior.
- The distinction between regular and chaotic behavior is fluid, with potential for transitions within orbits.