SCHEE, Jan and Zdeněk STUCHLÍK. Ultra-high-energy collisions in the superspinning Kerr geometry. Classical and Quantum Gravity. GB - Spojené království Velké Británie a, 2013, vol. 30, No 7, 25 pp. ISSN 0264-9381. Available from: https://dx.doi.org/10.1088/0264-9381/30/7/075012.
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Basic information
Original name Ultra-high-energy collisions in the superspinning Kerr geometry
Authors SCHEE, Jan and Zdeněk STUCHLÍK.
Edition Classical and Quantum Gravity, GB - Spojené království Velké Británie a, 2013, 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
WWW www
Organization unit Faculty of Philosophy and Science in Opava
Doi http://dx.doi.org/10.1088/0264-9381/30/7/075012
UT WoS 000316227500012
Keywords in English ROTATING BLACK-HOLE; NAKED-SINGULARITY; GRAVITATIONAL COLLAPSE
Tags UF
Tags International impact, Reviewed
Links GA202/09/0772, research and development project.
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 18/1/2021 13:56.
Abstract
Kerr naked singularities (superspinars) have to be efficiently converted to a black hole due to accretion from Keplerian discs. In the final stages of the conversion process the near-extreme Kerr naked singularities (superspinars) provide a variety of extraordinary physical phenomena. Such superspinning Kerr geometries can serve as an efficient accelerator for extremely high-energy collisions enabling direct and clear demonstration of the outcomes of the collision processes. We shall discuss the efficiency and visibility of the ultra-high-energy collisions in the deepest parts of the gravitational well of superspinning near-extreme Kerr geometries for the whole variety of particles freely falling from infinity. We demonstrate that the ultra-high-energyprocesses can be obtained with no fine tuning of the motion constants and the products of the collision can escape to infinity with both directional and energetical efficiency significantly higher than in the case of the near-extreme bla
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