HLEDÍK, Stanislav, Zdeněk STUCHLÍK and Kamila TRUPAROVÁ PLŠKOVÁ. Evolution of Kerr superspinars due to accretion counterrotating thin discs. Classical and Quantum Gravity. GB - Spojené království Velké Británie a, 2011, vol. 28, No 15, p. 1-23. ISSN 0264-9381. Available from: https://dx.doi.org/10.1088/0264-9381/28/15/155017.
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Basic information
Original name Evolution of Kerr superspinars due to accretion counterrotating thin discs
Authors HLEDÍK, Stanislav, Zdeněk STUCHLÍK and Kamila TRUPAROVÁ PLŠKOVÁ.
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/10.1088/0264-9381/28/15/155017
UT WoS 000292453000020
Keywords in English SUPERMASSIVE BLACK-HOLES, QUASI-PERIODIC OSCILLATIONS, ORBITAL RESONANCE MODEL, HIGH-FREQUENCY QPOS, NAKED-SINGULARITY, IRON LINE, COSMOLOGICAL CONSTANT, ENERGY EXTRACTION, MOLECULAR GAS, ALPHA LINES
Tags UF
Tags International impact, Reviewed
Links GA202/09/0772, research and development project. LC06014, research and development project. MSM4781305903, plan (intention).
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 8/12/2020 14:19.
Abstract
String theory predicts the existence of extremely compact objects spinning faster than Kerr black holes. The spacetime exterior to such superspinars is described by Kerr naked singularity geometry breaking the black-hole limit on the internal angular momentum. We demonstrate that the conversion of Kerr superspinars into a near-extreme black hole due to an accretion counterrotating Keplerian disc is much more effective in comparison with the case of a corotating one since both the accreted rest mass necessary for conversion and the evolution time of conversion are by orders smaller for counterrotating discs. The conversion time of Kerr superspinars is given for several accretion regimes, and it is shown that the self-regulated accretion flow implies fastest evolution to the black-hole state. In the final stages of the conversion, Kerr superspinars can serve as very efficient particle accelerators in the region where the black-hole horizon forms.
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