A relativistic bouncer on a vibrating surface

Detalhes bibliográficos
Autor(a) principal: Espinoza Ortiz, J. S.
Data de Publicação: 2018
Outros Autores: Lagos, R. E. [UNESP]
Tipo de documento: Artigo de conferência
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1088/1742-6596/1141/1/012113
http://hdl.handle.net/11449/188563
Resumo: We consider a special relativity scenario in order to study the dynamical behavior of a particle flying under the influence of a gravitational field, colliding successive times against a rigid vibrating surface, via a restitution coefficient. We define two re-scaled dimensionless dynamical variables, namely: the relative particle velocity W with respect to the surface's velocity, and the real parameter τ accounting for the temporal evolution of the system. In order to analyze the system's nonlinear dynamical behavior, we construct the mapping at the particle-surface contact point, described for the k'th collision, by the couple of variables (τ k Wk). Then, from the dynamical mapping, we compute the fixed point trajectory and analyze its stability. We find the dynamical behavior of the fixed point trajectory to be stable or unstable, according to the values of the re-scaled vibrating surface amplitude, the restitution coefficient and the auxiliary variable β G (0,1), sweeping from the non relativistic to the ultra relativistic regime. Other important dynamical aspects such as the phase space volume and the one cycle vibrating surface (decomposed into absorbing and transmitting regions) are also discussed. Furthermore, the model rescues well known results in the non relativistic limit.
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spelling A relativistic bouncer on a vibrating surfaceWe consider a special relativity scenario in order to study the dynamical behavior of a particle flying under the influence of a gravitational field, colliding successive times against a rigid vibrating surface, via a restitution coefficient. We define two re-scaled dimensionless dynamical variables, namely: the relative particle velocity W with respect to the surface's velocity, and the real parameter τ accounting for the temporal evolution of the system. In order to analyze the system's nonlinear dynamical behavior, we construct the mapping at the particle-surface contact point, described for the k'th collision, by the couple of variables (τ k Wk). Then, from the dynamical mapping, we compute the fixed point trajectory and analyze its stability. We find the dynamical behavior of the fixed point trajectory to be stable or unstable, according to the values of the re-scaled vibrating surface amplitude, the restitution coefficient and the auxiliary variable β G (0,1), sweeping from the non relativistic to the ultra relativistic regime. Other important dynamical aspects such as the phase space volume and the one cycle vibrating surface (decomposed into absorbing and transmitting regions) are also discussed. Furthermore, the model rescues well known results in the non relativistic limit.Departamento de Fisica Universidade Federal de GoiásDepartamento de Fisica IGCE UNESPDepartamento de Fisica IGCE UNESPUniversidade Federal de Goiás (UFG)Universidade Estadual Paulista (Unesp)Espinoza Ortiz, J. S.Lagos, R. E. [UNESP]2019-10-06T16:12:12Z2019-10-06T16:12:12Z2018-12-21info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjecthttp://dx.doi.org/10.1088/1742-6596/1141/1/012113Journal of Physics: Conference Series, v. 1141, n. 1, 2018.1742-65961742-6588http://hdl.handle.net/11449/18856310.1088/1742-6596/1141/1/0121132-s2.0-85059421300Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengJournal of Physics: Conference Seriesinfo:eu-repo/semantics/openAccess2021-10-22T21:54:10Zoai:repositorio.unesp.br:11449/188563Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T17:05:19.590023Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv A relativistic bouncer on a vibrating surface
title A relativistic bouncer on a vibrating surface
spellingShingle A relativistic bouncer on a vibrating surface
Espinoza Ortiz, J. S.
title_short A relativistic bouncer on a vibrating surface
title_full A relativistic bouncer on a vibrating surface
title_fullStr A relativistic bouncer on a vibrating surface
title_full_unstemmed A relativistic bouncer on a vibrating surface
title_sort A relativistic bouncer on a vibrating surface
author Espinoza Ortiz, J. S.
author_facet Espinoza Ortiz, J. S.
Lagos, R. E. [UNESP]
author_role author
author2 Lagos, R. E. [UNESP]
author2_role author
dc.contributor.none.fl_str_mv Universidade Federal de Goiás (UFG)
Universidade Estadual Paulista (Unesp)
dc.contributor.author.fl_str_mv Espinoza Ortiz, J. S.
Lagos, R. E. [UNESP]
description We consider a special relativity scenario in order to study the dynamical behavior of a particle flying under the influence of a gravitational field, colliding successive times against a rigid vibrating surface, via a restitution coefficient. We define two re-scaled dimensionless dynamical variables, namely: the relative particle velocity W with respect to the surface's velocity, and the real parameter τ accounting for the temporal evolution of the system. In order to analyze the system's nonlinear dynamical behavior, we construct the mapping at the particle-surface contact point, described for the k'th collision, by the couple of variables (τ k Wk). Then, from the dynamical mapping, we compute the fixed point trajectory and analyze its stability. We find the dynamical behavior of the fixed point trajectory to be stable or unstable, according to the values of the re-scaled vibrating surface amplitude, the restitution coefficient and the auxiliary variable β G (0,1), sweeping from the non relativistic to the ultra relativistic regime. Other important dynamical aspects such as the phase space volume and the one cycle vibrating surface (decomposed into absorbing and transmitting regions) are also discussed. Furthermore, the model rescues well known results in the non relativistic limit.
publishDate 2018
dc.date.none.fl_str_mv 2018-12-21
2019-10-06T16:12:12Z
2019-10-06T16:12:12Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/conferenceObject
format conferenceObject
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1088/1742-6596/1141/1/012113
Journal of Physics: Conference Series, v. 1141, n. 1, 2018.
1742-6596
1742-6588
http://hdl.handle.net/11449/188563
10.1088/1742-6596/1141/1/012113
2-s2.0-85059421300
url http://dx.doi.org/10.1088/1742-6596/1141/1/012113
http://hdl.handle.net/11449/188563
identifier_str_mv Journal of Physics: Conference Series, v. 1141, n. 1, 2018.
1742-6596
1742-6588
10.1088/1742-6596/1141/1/012113
2-s2.0-85059421300
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Journal of Physics: Conference Series
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.source.none.fl_str_mv Scopus
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
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