Numerical test of the method for revealing traces of deterministic chaos in the accreting black holes

The high energy radiation emitted by black hole X-ray binaries originates in an accretion disk, hence the variability of the lightcurves mirrors the dynamics of the disc. We study the time evolution of the emitted flux in order to find evidences, that low dimensional non-linear equations govern the...

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Autores principales: Suková, Petra, Janiuk, Agnieszk
Formato: Objeto de conferencia
Lenguaje:Inglés
Publicado: 2015
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/168114
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spelling I19-R120-10915-1681142024-07-29T20:01:56Z http://sedici.unlp.edu.ar/handle/10915/168114 Numerical test of the method for revealing traces of deterministic chaos in the accreting black holes Suková, Petra Janiuk, Agnieszk 2015-10 2016 2024-07-29T16:25:02Z en Ciencias Astronómicas accretion flow numerical time series chaotic behaviour The high energy radiation emitted by black hole X-ray binaries originates in an accretion disk, hence the variability of the lightcurves mirrors the dynamics of the disc. We study the time evolution of the emitted flux in order to find evidences, that low dimensional non-linear equations govern the accretion flow. Here we test the capabilities of our novel method to find chaotic behaviour on the two numerical time series describing the motion of a test particle around a black hole surrounded by a thin massive disc, one being regular and the other one chaotic. Facultad de Ciencias Astronómicas y Geofísicas Objeto de conferencia Objeto de conferencia http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf 179-182
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
accretion flow
numerical time series
chaotic behaviour
spellingShingle Ciencias Astronómicas
accretion flow
numerical time series
chaotic behaviour
Suková, Petra
Janiuk, Agnieszk
Numerical test of the method for revealing traces of deterministic chaos in the accreting black holes
topic_facet Ciencias Astronómicas
accretion flow
numerical time series
chaotic behaviour
description The high energy radiation emitted by black hole X-ray binaries originates in an accretion disk, hence the variability of the lightcurves mirrors the dynamics of the disc. We study the time evolution of the emitted flux in order to find evidences, that low dimensional non-linear equations govern the accretion flow. Here we test the capabilities of our novel method to find chaotic behaviour on the two numerical time series describing the motion of a test particle around a black hole surrounded by a thin massive disc, one being regular and the other one chaotic.
format Objeto de conferencia
Objeto de conferencia
author Suková, Petra
Janiuk, Agnieszk
author_facet Suková, Petra
Janiuk, Agnieszk
author_sort Suková, Petra
title Numerical test of the method for revealing traces of deterministic chaos in the accreting black holes
title_short Numerical test of the method for revealing traces of deterministic chaos in the accreting black holes
title_full Numerical test of the method for revealing traces of deterministic chaos in the accreting black holes
title_fullStr Numerical test of the method for revealing traces of deterministic chaos in the accreting black holes
title_full_unstemmed Numerical test of the method for revealing traces of deterministic chaos in the accreting black holes
title_sort numerical test of the method for revealing traces of deterministic chaos in the accreting black holes
publishDate 2015
url http://sedici.unlp.edu.ar/handle/10915/168114
work_keys_str_mv AT sukovapetra numericaltestofthemethodforrevealingtracesofdeterministicchaosintheaccretingblackholes
AT janiukagnieszk numericaltestofthemethodforrevealingtracesofdeterministicchaosintheaccretingblackholes
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