KOLOŠ, Martin and Zdeněk STUCHLÍK. Dynamics of current-carrying string loops in the Kerr naked-singularity and black-hole spacetimes. Physical Review D. US - Spojené státy americké, 2013, vol. 88, No 6. ISSN 1550-7998. Available from: https://dx.doi.org/10.1103/PhysRevD.88.065004.
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Basic information
Original name Dynamics of current-carrying string loops in the Kerr naked-singularity and black-hole spacetimes
Authors KOLOŠ, Martin and Zdeněk STUCHLÍK.
Edition Physical Review D, US - Spojené státy americké, 2013, 1550-7998.
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/10.1103/PhysRevD.88.065004
UT WoS 000323894000020
Keywords in English QUASI-PERIODIC OSCILLATIONS; X-RAY BINARIES; FLUX TUBES
Tags UF
Tags International impact, Reviewed
Links GA202/09/0772, research and development project.
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 26/1/2021 09:56.
Abstract
Current-carrying string-loop dynamics is studied in the Kerr spacetimes. With attention concentrated to the axisymmetric motion of string loops around the symmetry axis of both black-hole (BH) and naked singularity (NS) spacetimes, it is shown that the resulting motion is governed by the presence of an outer tension barrier and an inner angular momentum barrier that are influenced by the BH or NS spin. We classify the string dynamics according to properties of the energy boundary function (effective potential) for the string loop motion. We have found that for NS there exist new types of energy boundary function, namely those with off-equatorial minima. Conversion of the energy of the string oscillations to the energy of the linear translational motionhas been studied. Such a transmutation effect is much more efficient in the NS spacetimes because of lack of the event horizon. For BH spacetimes efficiency of the transmutation effect is only weakly spin dependent. Transition from the r
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