Shannon entropy applied to the planar restricted three-body problem

CINCOTTA, P. M.; BEAUGÉ, C

CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY

SPRINGER

Año: 2019 vol. 131

0923-2958

We present a numerical study of the application of the Shannon entropy technique to the planar restricted three-body problem in the vicinity of first-order interior mean-motion resonances with the perturber. We estimate the diffusion coefficient for a series of initial conditions andcompare the results with calculations obtained from the time evolution of the variance in the semimajor axis and eccentricity plane. Adopting adequate normalization factors, both methods yield comparable results, although much shorter integration times are required for entropy calculations. A second advantage of the use of entropy is that it is possible to obtain reliable results even without the use of ensembles or analysis restricted to surfaces of section or representative planes. This allows for a much more numerically efficient tool that may beincorporated into a working N-body code and applied to numerous dynamical problems in planetary dynamics. Finally, we estimate instability times for a series of initial conditions in the 2/1 and 3/2 mean-motion resonances and compare them with times of escape obtainedfrom directed N-body simulations. We find very good agreement in all cases, not only with respect to average values but also in their dispersion for nearby trajectories.