Diffusion phenomena in a mixed phase space
dc.contributor.author | Palmero, Matheus S. [UNESP] | |
dc.contributor.author | Díaz, Gabriel I. | |
dc.contributor.author | McClintock, Peter V. E. | |
dc.contributor.author | Leonel, Edson D. [UNESP] | |
dc.contributor.institution | Universidade Estadual Paulista (Unesp) | |
dc.contributor.institution | Lancaster University | |
dc.contributor.institution | Universidade de São Paulo (USP) | |
dc.date.accessioned | 2020-12-12T01:12:41Z | |
dc.date.available | 2020-12-12T01:12:41Z | |
dc.date.issued | 2020-01-01 | |
dc.description.abstract | We show that, in strongly chaotic dynamical systems, the average particle velocity can be calculated analytically by consideration of Brownian dynamics in a phase space, the method of images, and the use of the classical diffusion equation. The method is demonstrated on the simplified Fermi-Ulam accelerator model, which has a mixed phase space with chaotic seas, invariant tori, and Kolmogorov-Arnold-Moser islands. The calculated average velocities agree well with numerical simulations and with an earlier empirical theory. | en |
dc.description.affiliation | Departamento de Física UNESP - Univ Estadual Paulista, Av. 24A, 1515, Bela Vista | |
dc.description.affiliation | Department of Physics Lancaster University | |
dc.description.affiliation | Instituto de Física - Universidade de São Paulo (IFUSP) Cidade Universitária, Rua do Matão, Tr.R 187 | |
dc.description.affiliationUnesp | Departamento de Física UNESP - Univ Estadual Paulista, Av. 24A, 1515, Bela Vista | |
dc.identifier | http://dx.doi.org/10.1063/1.5100607 | |
dc.identifier.citation | Chaos, v. 30, n. 1, 2020. | |
dc.identifier.doi | 10.1063/1.5100607 | |
dc.identifier.issn | 1054-1500 | |
dc.identifier.scopus | 2-s2.0-85078254841 | |
dc.identifier.uri | http://hdl.handle.net/11449/198429 | |
dc.language.iso | eng | |
dc.relation.ispartof | Chaos | |
dc.source | Scopus | |
dc.title | Diffusion phenomena in a mixed phase space | en |
dc.type | Artigo | |
unesp.author.orcid | 0000-0003-3211-2560 0000-0003-3211-2560 0000-0003-3211-2560[1] |