2013
Ultra-high-energy collisions in the superspinning Kerr geometry
SCHEE, Jan and Zdeněk STUCHLÍKBasic information
Original name
Ultra-high-energy collisions in the superspinning Kerr geometry
Authors
Edition
Classical and Quantum Gravity, GB - Spojené království Velké Británie a, 2013, 0264-9381
Other information
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
References:
Impact factor
Impact factor: 3.103
Organization unit
Faculty of Philosophy and Science in Opava
UT WoS
000316227500012
EID Scopus
2-s2.0-84875276456
Keywords in English
ROTATING BLACK-HOLE; NAKED-SINGULARITY; GRAVITATIONAL COLLAPSE
Tags
Tags
International impact, Reviewed
Links
GA202/09/0772, research and development project.
Changed: 18/1/2021 13:56, Mgr. Pavlína Jalůvková
Abstract
In the original language
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