The Liapunov exponent as a tool for exploring phase space
Autor(a) principal: | |
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Data de Publicação: | 1996 |
Outros Autores: | , , , |
Tipo de documento: | Artigo de conferência |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1007/978-94-009-0307-4_20 http://hdl.handle.net/11449/33016 |
Resumo: | We have used the Liapunov exponent to explore the phase space of a dynamical system. Considering the planar, circular restricted three-body problem for a mass ratio mu = 10(-3) (close to the Jupiter/Sun case), we have integrated similar to 16,000 starting conditions for orbits started interior to that of the perturber and we have estimated the maximum Liapunov characteristic exponent for each starting condition. Despite the fact that the integrations, in general, are for only a few thousand orbital periods of the secondary, a comparative analysis of the Liapunov exponents for various values of the 'cut-off' gives a good overview of the structure of the phase space. It provides information about the diffusion rates of the various chaotic regions, the location of the regular regions associated with primary resonances and even details such as the location of secondary resonances that produce chaotic regions inside the regular regions of primary resonances. |
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The Liapunov exponent as a tool for exploring phase spacechaosLiapunov exponentsorbitsWe have used the Liapunov exponent to explore the phase space of a dynamical system. Considering the planar, circular restricted three-body problem for a mass ratio mu = 10(-3) (close to the Jupiter/Sun case), we have integrated similar to 16,000 starting conditions for orbits started interior to that of the perturber and we have estimated the maximum Liapunov characteristic exponent for each starting condition. Despite the fact that the integrations, in general, are for only a few thousand orbital periods of the secondary, a comparative analysis of the Liapunov exponents for various values of the 'cut-off' gives a good overview of the structure of the phase space. It provides information about the diffusion rates of the various chaotic regions, the location of the regular regions associated with primary resonances and even details such as the location of secondary resonances that produce chaotic regions inside the regular regions of primary resonances.UNESP,GRP DINAM ORBITAL & PLANETOL,CP 205,BR-12500000 GUARATINGUETA,SP,BRAZILUNESP,GRP DINAM ORBITAL & PLANETOL,CP 205,BR-12500000 GUARATINGUETA,SP,BRAZILKluwer Academic PublUniversidade Estadual Paulista (Unesp)Winter, O. C.Murray, C. D.Muzzio, J. C.FerrazMello, S.Henrard, J.2014-05-20T15:21:56Z2014-05-20T15:21:56Z1996-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObject215-219http://dx.doi.org/10.1007/978-94-009-0307-4_20Chaos In Gravitational N-body Systems. Dordrecht: Kluwer Academic Publ, p. 215-219, 1996.http://hdl.handle.net/11449/3301610.1007/978-94-009-0307-4_20WOS:A1996BG72A000200960024575647258Web of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengChaos In Gravitational N-body Systemsinfo:eu-repo/semantics/openAccess2024-07-02T14:29:49Zoai:repositorio.unesp.br:11449/33016Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T22:43:43.718294Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
The Liapunov exponent as a tool for exploring phase space |
title |
The Liapunov exponent as a tool for exploring phase space |
spellingShingle |
The Liapunov exponent as a tool for exploring phase space Winter, O. C. chaos Liapunov exponents orbits |
title_short |
The Liapunov exponent as a tool for exploring phase space |
title_full |
The Liapunov exponent as a tool for exploring phase space |
title_fullStr |
The Liapunov exponent as a tool for exploring phase space |
title_full_unstemmed |
The Liapunov exponent as a tool for exploring phase space |
title_sort |
The Liapunov exponent as a tool for exploring phase space |
author |
Winter, O. C. |
author_facet |
Winter, O. C. Murray, C. D. Muzzio, J. C. FerrazMello, S. Henrard, J. |
author_role |
author |
author2 |
Murray, C. D. Muzzio, J. C. FerrazMello, S. Henrard, J. |
author2_role |
author author author author |
dc.contributor.none.fl_str_mv |
Universidade Estadual Paulista (Unesp) |
dc.contributor.author.fl_str_mv |
Winter, O. C. Murray, C. D. Muzzio, J. C. FerrazMello, S. Henrard, J. |
dc.subject.por.fl_str_mv |
chaos Liapunov exponents orbits |
topic |
chaos Liapunov exponents orbits |
description |
We have used the Liapunov exponent to explore the phase space of a dynamical system. Considering the planar, circular restricted three-body problem for a mass ratio mu = 10(-3) (close to the Jupiter/Sun case), we have integrated similar to 16,000 starting conditions for orbits started interior to that of the perturber and we have estimated the maximum Liapunov characteristic exponent for each starting condition. Despite the fact that the integrations, in general, are for only a few thousand orbital periods of the secondary, a comparative analysis of the Liapunov exponents for various values of the 'cut-off' gives a good overview of the structure of the phase space. It provides information about the diffusion rates of the various chaotic regions, the location of the regular regions associated with primary resonances and even details such as the location of secondary resonances that produce chaotic regions inside the regular regions of primary resonances. |
publishDate |
1996 |
dc.date.none.fl_str_mv |
1996-01-01 2014-05-20T15:21:56Z 2014-05-20T15:21:56Z |
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/10.1007/978-94-009-0307-4_20 Chaos In Gravitational N-body Systems. Dordrecht: Kluwer Academic Publ, p. 215-219, 1996. http://hdl.handle.net/11449/33016 10.1007/978-94-009-0307-4_20 WOS:A1996BG72A00020 0960024575647258 |
url |
http://dx.doi.org/10.1007/978-94-009-0307-4_20 http://hdl.handle.net/11449/33016 |
identifier_str_mv |
Chaos In Gravitational N-body Systems. Dordrecht: Kluwer Academic Publ, p. 215-219, 1996. 10.1007/978-94-009-0307-4_20 WOS:A1996BG72A00020 0960024575647258 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Chaos In Gravitational N-body Systems |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
215-219 |
dc.publisher.none.fl_str_mv |
Kluwer Academic Publ |
publisher.none.fl_str_mv |
Kluwer Academic Publ |
dc.source.none.fl_str_mv |
Web of Science 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_ |
1808129454869839872 |