dc.creatorCincotta, Pablo Miguel
dc.creatorGiordano, Claudia Marcela
dc.creatorAlves Silva, Raphael
dc.creatorBeaugé, Cristián
dc.date2021-02
dc.date2022-11-07T13:56:12Z
dc.date.accessioned2023-07-15T05:00:15Z
dc.date.available2023-07-15T05:00:15Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/145267
dc.identifierissn:0923-2958
dc.identifierissn:1572-9478
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7471716
dc.descriptionIn the present effort, we revisit the Shannon entropy approach for the study of both the extent and the rate of diffusion in a given dynamical system. In particular, we provide a theoretical and numerical study of the dependence of the formulation on the parameters of the method. We succeed in deriving not only a diffusion coefficient, D<sub>S</sub>, but also an estimate of the macroscopical instability time for the system under study. Dealing with a toy model, namely a 4D symplectic application that represents the dynamics around a junction of resonances of different order, and an a particular case of the planar three-body problem, the HD20003 planetary system, we obtain numerical evidence that D<sub>S</sub> is a robust measure of the diffusion rate, no significant dependence on the free parameter of the entropy formulation (the size of the elements of the partition) being observed. Moreover, successful results concerning the estimation of macroscopical instability times obtained from D<sub>S</sub> are presented in both cases.
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.descriptionInstituto de Astrofísica de La Plata
dc.formatapplication/pdf
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by/4.0/
dc.rightsCreative Commons Attribution 4.0 International (CC BY 4.0)
dc.subjectAstronomía
dc.subjectChaotic diffusion
dc.subjectResonances
dc.subjectShannon entropy
dc.subjectThree-body problem
dc.titleShannon entropy diffusion estimates: sensitivity on the parameters of the method
dc.typeArticulo
dc.typeArticulo


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