Number of the records: 1
Effective potential of particles in the oblique black hole magnetosphere
- 1.
SYSNO ASEP 0484913 Document Type C - Proceedings Paper (int. conf.) R&D Document Type Conference Paper Title Effective potential of particles in the oblique black hole magnetosphere Author(s) Kopáček, Ondřej (ASU-R) RID, ORCID
Karas, Vladimír (ASU-R) RID, ORCIDSource Title Proceedings of the Fourteenth Marcel Grossmann Meeting on General Relativity, Accretion Processes onto Black Holes: Observation and Modeling, Part B. - Singapore : World Scientific Publishing, 2017 / Bianchi M. - ISBN 9789813226593 Pages s. 1050-1055 Number of pages 6 s. Publication form Print - P Action Marcel Grossmann Meeting on General Relativity /14./ Event date 12.06.2015 - 18.06.2015 VEvent location Rome Country IT - Italy Event type WRD Language eng - English Country SG - Singapore Keywords black holes ; magnetosphere ; non-axisymmetry Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics OECD category Astronomy (including astrophysics,space science) R&D Projects GB14-37086G GA ČR - Czech Science Foundation (CSF) Institutional support ASU-R - RVO:67985815 DOI 10.1142/9789813226609_0060 Annotation Dynamics of charged matter in the oblique black hole magnetosphere is investigated. In particular, we adopt a model consisting of a rotating black hole embedded in the external large-scale magnetic field that is inclined arbitrarily with respect to the rotation axis. Breaking the axial symmetry appears to have profound consequences regarding the dynamics of particles and it also poses some methodological difficulties. In this contribution we discuss the applicability of the method of effective potential for the non-axisymmetric model and show that it may only be applied in the appropriate reference frame. Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2018
Number of the records: 1