D 2020

Oscillations of non-slender tori in the Hartle-Thorne external geometry

MATUSZKOVÁ, Monika, Kateřina KLIMOVIČOVÁ, Gabriela URBANCOVÁ, Debora LANČOVÁ, Eva ŠRÁMKOVÁ et. al.

Basic information

Original name

Oscillations of non-slender tori in the Hartle-Thorne external geometry

Authors

MATUSZKOVÁ, Monika (203 Czech Republic, belonging to the institution), Kateřina KLIMOVIČOVÁ (203 Czech Republic, belonging to the institution), Gabriela URBANCOVÁ (203 Czech Republic, belonging to the institution), Debora LANČOVÁ (203 Czech Republic, belonging to the institution), Eva ŠRÁMKOVÁ (203 Czech Republic, belonging to the institution) and Gabriel TÖRÖK (203 Czech Republic, belonging to the institution)

Edition

Opava, Proceedings of RAGtime 22: Workshops on black holes and neutron stars, p. 185-201, 17 pp. 2020

Publisher

Slezská univerzita v Opavě, Fyzikální ústav v Opavě

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:

URL

RIV identification code

RIV/47813059:19630/20:A0000049

Organization unit

Institute of physics in Opava

ISBN

978-80-7510-432-8

ISSN

Keywords in English

neutron star; thick accretion disc; Hartle-Thorne metric

Tags

EF18_0540014696, EF19_073-0016951, , FÚ2020, LTI17018, LTT17003, RAGtime 22, RIV21, SGF-1-2020, SGS12-2019, SGS13-2019

Tags

International impact

Links

EF18_054/0014696, research and development project. EF19_073/0016951, research and development project. LTI17018, research and development project. LTT17003, research and development project.
Změněno: 13/9/2022 08:56, Mgr. Pavlína Jalůvková

Abstract

V originále

We examine the influence of the quadrupole moment of a slowly rotating neutronstar on the oscillations of non-slender accretion tori. We apply previously developedmethods to perform analytical calculations of frequencies of the radial epicyclicmode of a torus in the specific case of the Hartle-Thorne geometry. We presenthere our preliminary results and provide a brief comparison between the calculated frequencies and the frequencies previously obtained assuming both standard and lin-earized Kerr geometry. Finally, we shortly discuss the consequences for models of high-frequency quasi-periodic oscillations observed in low-mass X-ray binaries.
Displayed: 24/12/2024 04:10