KOVÁŘ, Jiří, Vladimír KARAS, Yasufumi KOJIMA and Ondřej KOPÁČEK. Regular and chaotic orbits near a massive magnetic dipole. Classical and Quantum Gravity. GB - Spojené království Velké Británie a, 2013, vol. 30, No 2, p. '025010-1'-'025010-23', 23 pp. ISSN 0264-9381. Available from: https://dx.doi.org/10.1088/0264-9381/30/2/025010.
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Basic information
Original name Regular and chaotic orbits near a massive magnetic dipole
Authors KOVÁŘ, Jiří, Vladimír KARAS, Yasufumi KOJIMA and Ondřej KOPÁČEK.
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/10.1088/0264-9381/30/2/025010
UT WoS 000313097300010
Keywords in English magnetic dipole;chaotic orbits;regular orbits;Bonnor spacetime;off-equatorial trajectories;particle motion
Tags UF
Tags International impact, Reviewed
Links EE2.3.20.0071, research and development project. GPP209/10/P190, research and development project.
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 15/2/2021 10:18.
Abstract
Within the framework of Bonnor's exact solution describing a massive magnetic dipole, we study the motion of neutral and electrically charged test particles. In dependence on the Bonnor spacetime parameters, we determine regions enabling the existence of stable circular orbits confined to the equatorial plane and of those levitating above the equatorial plane. Constructing Poincare surfaces of section and recurrence plots, we also investigate the dynamics of particles moving along general off-equatorial trajectories bound in effective potential wells forming around the stable circular orbits. We demonstrate that the motion in the Bonnor spacetime is not integrable. This extends previous investigations of generalized Stormer's problem into the realm of exact solutions of Einstein-Maxwell equations, where the gravitational and electromagnetic effects play a comparable role on the particle motion.
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