Detailed Information on Publication Record
2017
Epicyclic oscillations of thick relativistic disks
HORÁK, Jiří, Odelle STRAUB, Eva ŠRÁMKOVÁ, Kateřina GOLUCHOVÁ, Gabriel TÖRÖK et. al.Basic information
Original name
Epicyclic oscillations of thick relativistic disks
Authors
HORÁK, Jiří (203 Czech Republic), Odelle STRAUB (756 Switzerland), Eva ŠRÁMKOVÁ (203 Czech Republic, guarantor, belonging to the institution), Kateřina GOLUCHOVÁ (203 Czech Republic, belonging to the institution) and Gabriel TÖRÖK (203 Czech Republic, belonging to the institution)
Edition
1. vyd. Opava (Česká republika), Proceedings of RAGtime 17–19: Workshops on black holes and neutron stars, 17–19/23–26 Oct., 1–5 Nov. 2015/2016/2017, Opava, Czech Republic, p. 47-59, 13 pp. 2017
Publisher
Slezská univerzita v Opavě, Filozoficko–přírodovědecká fakulta v Opavě, Ústav fyziky
Other information
Language
English
Type of outcome
Stať ve sborníku
Field of Study
10308 Astronomy
Country of publisher
Czech Republic
Confidentiality degree
není předmětem státního či obchodního tajemství
Publication form
printed version "print"
References:
RIV identification code
RIV/47813059:19240/17:A0000040
Organization unit
Faculty of Philosophy and Science in Opava
ISBN
978-80-7510-256-0
ISSN
Keywords in English
black hole physics; accretion disks; oscillations; FEM method
Tags
International impact, Reviewed
Links
GA17-16287S, research and development project.
Změněno: 6/4/2018 17:37, RNDr. Jan Hladík, Ph.D.
Abstract
V originále
We study epicyclic oscillations of thick relativistic tori with constant specific angular momentum distribution using the finite element numerical method. We have compared frequencies of the axisymmetric and non-axisymmetric modes with the analytic formulae obtained by Straub and Šrámková (2009) and Fragile et al. (2016). We have found excellent agreement in the case of axisymmetric radial epicyclic modes. In the case of the axisymmetric vertical epicyclic modes and non-axisymmetric modes in general, the analytic approximation agrees with numerical results only for tori of moderate thicknesses. Our analysis also revealed an instability of the thick constant angular momentum tori with respect to the radial epicyclic oscillations.