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dc.date.accessioned 2024-07-29T16:25:02Z
dc.date.available 2024-07-29T16:25:02Z
dc.date.issued 2016
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/168114
dc.description.abstract 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. en
dc.format.extent 179-182 es
dc.language en es
dc.subject accretion flow es
dc.subject numerical time series es
dc.subject chaotic behaviour es
dc.title Numerical test of the method for revealing traces of deterministic chaos in the accreting black holes en
dc.type Objeto de conferencia es
sedici.identifier.isbn 978-987-24948-3-4 es
sedici.creator.person Suková, Petra es
sedici.creator.person Janiuk, Agnieszk es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Objeto de conferencia es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.date.exposure 2015-10
sedici.relation.event High-Energy Phenomena tn Relativistic Outflows V (La Plata, 5 al 8 de octubre de 2015) es
sedici.description.peerReview peer-review es
sedici.relation.isRelatedWith https://sedici.unlp.edu.ar/handle/10915/167830 es
sedici.relation.bookTitle Proceedings of the High-Energy Phenomena in Relativistic Outflows V meeting es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)