Physics
Scientific paper
Jul 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phrva..46..837r&link_type=abstract
Physical Review A (ISSN 1050-2947), vol. 46, no. 2, July 15, 1992, p. 837-843. Research supported by Robert A. Welch Foundation
Physics
19
Gravitation Theory, Gravitational Fields, Orbital Mechanics, Ergodic Process, Gravitational Effects, Many Body Problem
Scientific paper
The failure of the one-dimensional gravitational system to relax to equilibrium on predicted time scales has raised questions concerning the ergodic properties of the dynamics. A failure to approach equilibrium could be caused by the segmentation of phase space into isolated regions from which the system cannot escape. In general, each region may have distinct ergodic properties. By numerically investigating the stability of two classes of periodic orbits for the N-body system, it is demonstrated that stable regions in the phase space exist for values of N of not more than 10. For populations of N between 11 and 20 inclusive numerical evidence is found for multiple chaotic invariant regions. Thus the failure of large systems (N of at least 100) to equilibrate may be a result of microscopic dynamical restrictions rather than imposed macroscopic constraints.
Miller Bruce N.
Reidl Charles J. Jr.
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