BLASCHKE, Martin, Petr SLANÝ and Zdeněk STUCHLÍK. Non-monotonic Keplerian velocity profiles around near-extreme braneworld Kerr black holes. Classical and Quantum Gravity. GB - Spojené království Velké Británie a, 2011, vol. 28, No 17, 18 pp. ISSN 0264-9381. Available from: https://dx.doi.org/10.1088/0264-9381/28/17/175002.
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Basic information
Original name Non-monotonic Keplerian velocity profiles around near-extreme braneworld Kerr black holes
Authors BLASCHKE, Martin, Petr SLANÝ and Zdeněk STUCHLÍK.
Edition Classical and Quantum Gravity, GB - Spojené království Velké Británie a, 2011, 0264-9381.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Confidentiality degree is not subject to a state or trade secret
Organization unit Faculty of Philosophy and Science in Opava
Doi http://dx.doi.org/10.1088/0264-9381/28/17/175002
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 UF
Tags International impact, Reviewed
Links LC06014, research and development project. MSM4781305903, plan (intention).
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 13/1/2021 11:38.
Abstract
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
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