Numerical test of the method for revealing traces of deterministic chaos in the accreting black holes
- Autores
- Suková, Petra; Janiuk, Agnieszk
- Año de publicación
- 2015
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- 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 - Materia
-
Ciencias Astronómicas
accretion flow
numerical time series
chaotic behaviour - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/168114
Ver los metadatos del registro completo
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Numerical test of the method for revealing traces of deterministic chaos in the accreting black holesSuková, PetraJaniuk, AgnieszkCiencias Astronómicasaccretion flownumerical time serieschaotic behaviourThe 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 Geofísicas2015-10info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionObjeto de conferenciahttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdf179-182http://sedici.unlp.edu.ar/handle/10915/168114enginfo:eu-repo/semantics/altIdentifier/isbn/978-987-24948-3-4info:eu-repo/semantics/reference/url/https://sedici.unlp.edu.ar/handle/10915/167830info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:44:50Zoai:sedici.unlp.edu.ar:10915/168114Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:44:51.002SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Numerical test of the method for revealing traces of deterministic chaos in the accreting black holes |
title |
Numerical test of the method for revealing traces of deterministic chaos in the accreting black holes |
spellingShingle |
Numerical test of the method for revealing traces of deterministic chaos in the accreting black holes Suková, Petra Ciencias Astronómicas accretion flow numerical time series chaotic behaviour |
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 |
dc.creator.none.fl_str_mv |
Suková, Petra Janiuk, Agnieszk |
author |
Suková, Petra |
author_facet |
Suková, Petra Janiuk, Agnieszk |
author_role |
author |
author2 |
Janiuk, Agnieszk |
author2_role |
author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas accretion flow numerical time series chaotic behaviour |
topic |
Ciencias Astronómicas accretion flow numerical time series chaotic behaviour |
dc.description.none.fl_txt_mv |
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 |
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. |
publishDate |
2015 |
dc.date.none.fl_str_mv |
2015-10 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/conferenceObject info:eu-repo/semantics/publishedVersion Objeto de conferencia http://purl.org/coar/resource_type/c_5794 info:ar-repo/semantics/documentoDeConferencia |
format |
conferenceObject |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://sedici.unlp.edu.ar/handle/10915/168114 |
url |
http://sedici.unlp.edu.ar/handle/10915/168114 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/isbn/978-987-24948-3-4 info:eu-repo/semantics/reference/url/https://sedici.unlp.edu.ar/handle/10915/167830 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
dc.format.none.fl_str_mv |
application/pdf 179-182 |
dc.source.none.fl_str_mv |
reponame:SEDICI (UNLP) instname:Universidad Nacional de La Plata instacron:UNLP |
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SEDICI (UNLP) |
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SEDICI (UNLP) |
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Universidad Nacional de La Plata |
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UNLP |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
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alira@sedici.unlp.edu.ar |
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