The Relative Lyapunov Indicators: Theory and Application to Dynamical Astronomy
Fil: Sandor, Zsolt. Konkoly Observatory of the Hungarian Academy of Sciences; Hungría.
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2015
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Acceso en línea: | https://rid.unrn.edu.ar/jspui/handle/20.500.12049/3766 https://doi.org/10.1007/978-3-662-48410-4_6 |
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I65-R171-20.500.12049-37662023-05-18T17:12:30Z application/pdf info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/4.0/ 2015-01 Fil: Sandor, Zsolt. Konkoly Observatory of the Hungarian Academy of Sciences; Hungría. Fil: Maffione, Nicolás P. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Grupo de Caos en Sistemas Hamiltonianos; Argentina The Relative Lyapunov Indicators: Theory and Application to Dynamical Astronomy Sandor, Zsolt Maffione, Nicolás Pablo Planetary System Giant Planet Chaotic Orbit Regular Orbit Dark Matter Halo true 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. Sándor Z., Maffione N. (2016) The Relative Lyapunov Indicators: Theory and Application to Dynamical Astronomy. In: Skokos C., Gottwald G., Laskar J. (eds) Chaos Detection and Predictability. Lecture Notes in Physics, vol 915. Springer, Berlin, Heidelberg 0075-8450 https://rid.unrn.edu.ar/jspui/handle/20.500.12049/3766 https://doi.org/10.1007/978-3-662-48410-4_6 en 915 Lecture Notes in Physics Springer |
institution |
Universidad Nacional de Río Negro |
institution_str |
I-65 |
repository_str |
R-171 |
collection |
Repositorio Institucional Digital de la Universidad Nacional de Río Negro (UNRN) |
language |
Inglés |
orig_language_str_mv |
en |
topic |
Planetary System Giant Planet Chaotic Orbit Regular Orbit Dark Matter Halo |
spellingShingle |
Planetary System Giant Planet Chaotic Orbit Regular Orbit Dark Matter Halo Sandor, Zsolt Maffione, Nicolás Pablo The Relative Lyapunov Indicators: Theory and Application to Dynamical Astronomy |
topic_facet |
Planetary System Giant Planet Chaotic Orbit Regular Orbit Dark Matter Halo |
description |
Fil: Sandor, Zsolt. Konkoly Observatory of the Hungarian Academy of Sciences; Hungría. |
author |
Sandor, Zsolt Maffione, Nicolás Pablo |
author_facet |
Sandor, Zsolt Maffione, Nicolás Pablo |
author_sort |
Sandor, Zsolt |
title |
The Relative Lyapunov Indicators: Theory and Application to Dynamical Astronomy |
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 |
relative lyapunov indicators: theory and application to dynamical astronomy |
publisher |
Springer |
publishDate |
2015 |
url |
https://rid.unrn.edu.ar/jspui/handle/20.500.12049/3766 https://doi.org/10.1007/978-3-662-48410-4_6 |
work_keys_str_mv |
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