D 2007

Orbital resonance model of QPOs in braneworld Kerr black hole spacetimes

KOTRLOVÁ, Andrea and zdenek STUCHLIK

Basic information

Original name

Orbital resonance model of QPOs in braneworld Kerr black hole spacetimes

Authors

KOTRLOVÁ, Andrea and zdenek STUCHLIK

Edition

Opava, Proceedings of RAGtime 8/9: Workshops on black holes and neutron stars, p. 323-361, 38 pp. 2007

Publisher

Slezská univerzita v Opavě, Filozoficko-přírodovědecká fakulta, 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

Organization unit

Faculty of Philosophy and Science in Opava

ISBN

978-80-7248-419-5

Keywords in English

Accretion, accretion discs, braneworld black hole physics, X-rays: general

Tags

Tags

International impact

Links

GA202/06/0041, research and development project. GD205/03/H144, research and development project. LC06014, research and development project. MSM4781305903, plan (intention).
Změněno: 10/12/2020 08:48, Mgr. Pavlína Jalůvková

Abstract

V originále

We investigate the role of the tidal charge in the orbital resonance model of quasiperiodic oscillations (QPOs) in black hole systems. The orbital Keplerian frequency and the radial and vertical epicyclic frequencies of the equatorial, quasicircular geodetical motion are discussed, and the local maxima of their radial profiles related to Keplerian accretion discs are given, assuming the inner edge of the disc located at loci of the innermost stable circular geodesic. It is shown, how the tidal charge could influence matching of the observational data indicating the 3:2 frequency ratio observed in GRS 1915+105 microquasar with prediction of the orbital resonance model.