A relativistic bouncer on a vibrating surface
Autor(a) principal: | |
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Data de Publicação: | 2018 |
Outros Autores: | |
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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Repositório Institucional da UNESP |
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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) |
repository.mail.fl_str_mv |
|
_version_ |
1808128753833869312 |