The relative Lyapunov indicators: Theory and application to dynamical astronomy
- Autores
- Sándor, Zsolt; Maffione, Nicolas Pablo
- Año de publicación
- 2016
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- A recently introduced chaos detection method, the Relative Lyapunov Indicator (RLI) is investigated in the cases of symplectic mappings and continuous Hamiltonian systems. It is shown that the RLI is an efficient numerical tool in determining the true nature of individual orbits, and in separating ordered and chaotic regions of the phase space of dynamical systems. A comparison between the RLI and some other variational indicators are presented, as well as the recent applications of the RLI to various problems of dynamical astronomy.
Fil: Sándor, Zsolt. Hungarian Academy of Sciences; Hungría
Fil: Maffione, Nicolas Pablo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina - Materia
-
RLI
Planetary System
Giant Planet
Chaotic Orbit
Regular Orbit
Dark Matter Halo
Relative Lyapunov Indicator
Hamiltonian systems - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-nd/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/97119
Ver los metadatos del registro completo
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The relative Lyapunov indicators: Theory and application to dynamical astronomySándor, ZsoltMaffione, Nicolas PabloRLIPlanetary SystemGiant PlanetChaotic OrbitRegular OrbitDark Matter HaloRelative Lyapunov IndicatorHamiltonian systemshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1A recently introduced chaos detection method, the Relative Lyapunov Indicator (RLI) is investigated in the cases of symplectic mappings and continuous Hamiltonian systems. It is shown that the RLI is an efficient numerical tool in determining the true nature of individual orbits, and in separating ordered and chaotic regions of the phase space of dynamical systems. A comparison between the RLI and some other variational indicators are presented, as well as the recent applications of the RLI to various problems of dynamical astronomy.Fil: Sándor, Zsolt. Hungarian Academy of Sciences; HungríaFil: Maffione, Nicolas Pablo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaSpringer2016-03info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/97119Sándor, Zsolt; Maffione, Nicolas Pablo; The relative Lyapunov indicators: Theory and application to dynamical astronomy; Springer; Lecture Notes In Physics; 915; 3-2016; 183-2200075-8450CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1007/978-3-662-48410-4_6info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/chapter/10.1007%2F978-3-662-48410-4_6info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1501.07264info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-nd/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:59:52Zoai:ri.conicet.gov.ar:11336/97119instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-22 11:59:52.39CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
The relative Lyapunov indicators: Theory and application to dynamical astronomy |
title |
The relative Lyapunov indicators: Theory and application to dynamical astronomy |
spellingShingle |
The relative Lyapunov indicators: Theory and application to dynamical astronomy Sándor, Zsolt RLI Planetary System Giant Planet Chaotic Orbit Regular Orbit Dark Matter Halo Relative Lyapunov Indicator Hamiltonian systems |
title_short |
The relative Lyapunov indicators: Theory and application to dynamical astronomy |
title_full |
The relative Lyapunov indicators: Theory and application to dynamical astronomy |
title_fullStr |
The relative Lyapunov indicators: Theory and application to dynamical astronomy |
title_full_unstemmed |
The relative Lyapunov indicators: Theory and application to dynamical astronomy |
title_sort |
The relative Lyapunov indicators: Theory and application to dynamical astronomy |
dc.creator.none.fl_str_mv |
Sándor, Zsolt Maffione, Nicolas Pablo |
author |
Sándor, Zsolt |
author_facet |
Sándor, Zsolt Maffione, Nicolas Pablo |
author_role |
author |
author2 |
Maffione, Nicolas Pablo |
author2_role |
author |
dc.subject.none.fl_str_mv |
RLI Planetary System Giant Planet Chaotic Orbit Regular Orbit Dark Matter Halo Relative Lyapunov Indicator Hamiltonian systems |
topic |
RLI Planetary System Giant Planet Chaotic Orbit Regular Orbit Dark Matter Halo Relative Lyapunov Indicator Hamiltonian systems |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
A recently introduced chaos detection method, the Relative Lyapunov Indicator (RLI) is investigated in the cases of symplectic mappings and continuous Hamiltonian systems. It is shown that the RLI is an efficient numerical tool in determining the true nature of individual orbits, and in separating ordered and chaotic regions of the phase space of dynamical systems. A comparison between the RLI and some other variational indicators are presented, as well as the recent applications of the RLI to various problems of dynamical astronomy. Fil: Sándor, Zsolt. Hungarian Academy of Sciences; Hungría Fil: Maffione, Nicolas Pablo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina |
description |
A recently introduced chaos detection method, the Relative Lyapunov Indicator (RLI) is investigated in the cases of symplectic mappings and continuous Hamiltonian systems. It is shown that the RLI is an efficient numerical tool in determining the true nature of individual orbits, and in separating ordered and chaotic regions of the phase space of dynamical systems. A comparison between the RLI and some other variational indicators are presented, as well as the recent applications of the RLI to various problems of dynamical astronomy. |
publishDate |
2016 |
dc.date.none.fl_str_mv |
2016-03 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/97119 Sándor, Zsolt; Maffione, Nicolas Pablo; The relative Lyapunov indicators: Theory and application to dynamical astronomy; Springer; Lecture Notes In Physics; 915; 3-2016; 183-220 0075-8450 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/97119 |
identifier_str_mv |
Sándor, Zsolt; Maffione, Nicolas Pablo; The relative Lyapunov indicators: Theory and application to dynamical astronomy; Springer; Lecture Notes In Physics; 915; 3-2016; 183-220 0075-8450 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1007/978-3-662-48410-4_6 info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/chapter/10.1007%2F978-3-662-48410-4_6 info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1501.07264 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-nd/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-nd/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
Springer |
publisher.none.fl_str_mv |
Springer |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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1846782321561174016 |
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12.982451 |