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dc.date.accessioned 2020-04-16T21:16:23Z
dc.date.available 2020-04-16T21:16:23Z
dc.date.issued 2018-11
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/93607
dc.description.abstract In the present work, we investigate phase correlations by recourse to the Shannon entropy. Using theoretical arguments, we show that the entropy provides an accurate measure of phase correlations in any dynamical system, in particular when dealing with a chaotic diffusion process. We apply this approach to different low-dimensional maps in order to show that indeed the entropy is very sensitive to the presence of correlations among the successive values of angular variables, even when it is weak. Later on, we apply this approach to unveil strong correlations in the time evolution of the phases involved in the Arnold’s Hamiltonian that lead to anomalous diffusion, particularly when the perturbation parameters are comparatively large. The obtained results allow us to discuss the validity of several approximations and assumptions usually introduced to derive a local diffusion coefficient in multidimensional near-integrable Hamiltonian systems, in particular the so-called reduced stochasticity approximation. en
dc.format.extent 1-17 es
dc.language en es
dc.subject Shannon Entropy es
dc.subject Diffusion es
dc.subject Phase correlations es
dc.title Phase correlations in chaotic dynamics: a Shannon entropy measure en
dc.type Articulo es
sedici.identifier.uri https://link.springer.com/article/10.1007%2Fs10569-018-9871-3 es
sedici.identifier.other https://doi.org/10.1007/s10569-018-9871-3 es
sedici.identifier.other hdl:11336/82434 es
sedici.identifier.issn 0923-2958 es
sedici.creator.person Cincotta, Pablo Miguel es
sedici.creator.person Giordano, Claudia Marcela es
sedici.subject.materias Astronomía es
sedici.subject.materias Física es
sedici.subject.materias Ciencias Naturales es
sedici.subject.materias Ciencias Exactas es
sedici.description.fulltext true es
mods.originInfo.place Instituto de Astrofísica de La Plata es
sedici.subtype Preprint es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Argentina (CC BY-NC-SA 2.5)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/2.5/ar/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Celestial Mechanics & Dynamical Astronomy es
sedici.relation.journalVolumeAndIssue vol. 130, no. 74 es


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Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Argentina (CC BY-NC-SA 2.5) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Argentina (CC BY-NC-SA 2.5)