id I65-R171-20.500.12049-2869
record_format dspace
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 Español
orig_language_str_mv es
topic Astronomía
Methods
Numerical
Galaxies
kinematics
Dynamics
Astronomía
spellingShingle Astronomía
Methods
Numerical
Galaxies
kinematics
Dynamics
Astronomía
Maffione, Nicolás Pablo
Darriba, Luciano A.
Cincotta, Pablo M.
Giordano, Claudia M.
Chaos detection tools
topic_facet Astronomía
Methods
Numerical
Galaxies
kinematics
Dynamics
Astronomía
description Fil: Maffione, Nicolas P. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata; Argentina
author Maffione, Nicolás Pablo
Darriba, Luciano A.
Cincotta, Pablo M.
Giordano, Claudia M.
author_facet Maffione, Nicolás Pablo
Darriba, Luciano A.
Cincotta, Pablo M.
Giordano, Claudia M.
author_sort Maffione, Nicolás Pablo
title Chaos detection tools
title_short Chaos detection tools
title_full Chaos detection tools
title_fullStr Chaos detection tools
title_full_unstemmed Chaos detection tools
title_sort chaos detection tools
publishDate 2012
url http://arxiv.org/abs/1212.3175
http://mnras.oxfordjournals.org/content/429/3/2700.abstract
http://hdl.handle.net/11336/3411
https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2869
http://dx.doi.org/10.1093/mnras/sts539
work_keys_str_mv AT maffionenicolaspablo chaosdetectiontools
AT darribalucianoa chaosdetectiontools
AT cincottapablom chaosdetectiontools
AT giordanoclaudiam chaosdetectiontools
AT maffionenicolaspablo applicationtoaselfconsistenttriaxialmodel
AT darribalucianoa applicationtoaselfconsistenttriaxialmodel
AT cincottapablom applicationtoaselfconsistenttriaxialmodel
AT giordanoclaudiam applicationtoaselfconsistenttriaxialmodel
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spelling I65-R171-20.500.12049-28692023-05-18T17:10:04Z application/pdf info:eu-repo/semantics/restrictedAccess https://creativecommons.org/licenses/by-nc-sa/4.0/ 2012-12-14 Fil: Maffione, Nicolas P. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata; Argentina Fil: Maffione, Nicolas P. Instituto de Astrofísica de La Plata; Argentina. Fil: Maffione, Nicolas P. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Darriba, Luciano A. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata; Argentina Fil: Darriba, Luciano A. Instituto de Astrofísica de La Plata; Argentina. Fil: Darriba, Luciano A. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Cincotta, Pablo M. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata; Argentina Fil: Cincotta, Pablo M. Instituto de Astrofísica de La Plata; Argentina. Fil: Cincotta, Pablo M. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Giordano, Claudia M. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata; Argentina Fil: Giordano, Claudia M. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Giordano, Claudia M. Instituto de Astrofísica de La Plata; Argentina. Chaos detection tools Application to a self-consistent triaxial model Maffione, Nicolás Pablo Darriba, Luciano A. Cincotta, Pablo M. Giordano, Claudia M. Astronomía Methods Numerical Galaxies kinematics Dynamics Astronomía true Together with the variational indicators of chaos, the spectral analysis methods have also achieved great popularity in the field of chaos detection. The former are based on the concept of local exponential divergence. The latter are based on the numerical analysis of some particular quantities of a single orbit, e.g. its frequency. In spite of having totally different conceptual bases, they are used for the very same goals such as, for instance, separating the chaotic and the regular component. In fact, we show herein that the variational indicators serve to distinguish both components of a Hamiltonian system in a more reliable fashion than a spectral analysis method does. We study two start spaces for different energy levels of a self? consistent triaxial stellar dynamical model by means of some selected variational indicators and a spectral analysis method. In order to select the appropriate tools for this paper, we extend previous studies where we make a comparison of several variational indicators on different scenarios. Herein, we compare the Average Power Law Exponent (APLE) and an alternative quantity given by the Mean Exponential Growth factor of Neary Orbits (MEGNO): the MEGNO? Slope Estimation of the largest Lyapunov Characteristic Exponent (SElLCE). The spectral analysis method selected for the investigation is the Frequency Modified Fourier Transform (FMFT). Besides a comparative study of the APLE, the Fast Lyapunov Indicator (FLI), the Orthogonal Fast Lyapunov Indicator (OFLI) and the MEGNO/SElLCE, we show that the SElLCE could be an appropriate alternative to the MEGNO when studying large samples of initial conditions. The SElLCE separates the chaotic and the regular components reliably and identifies the different levels of chaoticity. We show that the FMFT is not as reliable as the SElLCE to describe clearly the chaotic domains in the experiments. We use the latter indicator as the main variational indicator to analyse the phase space portraits of the model under study. Maffione, Nicolas P., Darriba, Luciano A., Cincotta, Pablo M. & Giordano, Claudia M. (2012). Chaos detection tools: application to a self-consistent triaxial model. Oxford University. Monthly Notices of the Royal Astronomical Society; 429; 3; pp. 2700-2717 0035-8711 http://arxiv.org/abs/1212.3175 http://mnras.oxfordjournals.org/content/429/3/2700.abstract http://hdl.handle.net/11336/3411 https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2869 http://dx.doi.org/10.1093/mnras/sts539 es 429 Monthly Notices of the Royal Astronomical Society