J 2011

Non-monotonic Keplerian velocity profiles around near-extreme braneworld Kerr black holes

BLASCHKE, Martin, Petr SLANÝ and Zdeněk STUCHLÍK

Basic information

Original name

Non-monotonic Keplerian velocity profiles around near-extreme braneworld Kerr black holes

Edition

Classical and Quantum Gravity, GB - Spojené království Velké Británie a, 2011, 0264-9381

Other information

Language

English

Type of outcome

Článek v odborném periodiku

Field of Study

10308 Astronomy

Confidentiality degree

není předmětem státního či obchodního tajemství

Organization unit

Faculty of Philosophy and Science in Opava

UT WoS

000294011800003

Keywords in English

QUASI-PERIODIC OSCILLATIONS, ORBITAL RESONANCE MODEL, HIGH-FREQUENCY QPOS, SGR-A-ASTERISK, NAKED SINGULARITY, GALAXY MCG-6-30-15, SPIN, MASS, ACCRETION, FIELD

Tags

Tags

International impact, Reviewed

Links

LC06014, research and development project. MSM4781305903, plan (intention).
Změněno: 13/1/2021 11:38, Mgr. Pavlína Jalůvková

Abstract

V originále

We study the non-monotonic Keplerian velocity profiles related to locally non-rotating frames (LNRF) in the field of near-extreme braneworld Kerr black holes and naked singularities in which the non-local gravitational effects of the bulk are representedby a braneworld tidal charge b and the 4D geometry of the spacetime structure is governed by the Kerr-Newman geometry. We show that positive tidal charge has a tendency to restrict the values of the black hole dimensionless spin a admitting the existence of the non-monotonic Keplerian LNRF-velocity profiles; the non-monotonic profiles exist in the black hole spacetimes with tidal charge smaller than b = 0.410 05 (and spin larger than a = 0.768 08). With decreasing value of the tidal charge (which neednot be only positive), both the region of spin allowing the non-monotonicity in the LNRF-velocity profile around braneworld Kerr black hole and the velocity difference in the minimum-maximum parts of the velocity profile increase implying