Particle Motion and Electromagnetic Fields of Rotating Compact Gravitating Objects with Gravitomagnetic Charge

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dc.creatorAbdujabbarov, A. A.
dc.creatorAhmedov, B. J.
dc.creatorKagramanova, V. G.
dc.date2008-02-29
dc.date2008-03-11
dc.date.accessioned2026-07-07T12:14:14Z
dc.date.available2026-07-07T12:14:14Z
dc.descriptionThe exact solution for the electromagnetic field occuring when the Kerr-Taub-NUT compact object is immersed (i) in an originally uniform magnetic field aligned along the axis of axial symmetry (ii) in dipolar magnetic field generated by current loop has been investigated. Effective potential of motion of charged test particle around Kerr-Taub-NUT gravitational source immersed in magnetic field with different values of external magnetic field and NUT parameter has been also investigated. In both cases presence of NUT parameter and magnetic field shifts stable circular orbits in the direction of the central gravitating object. Finally we find analytical solutions of Maxwell equations in the external background spacetime of a slowly rotating magnetized NUT star. The star is considered isolated and in vacuum, with monopolar configuration model for the stellar magnetic field.
dc.description18 pages, 6 figures, new results in section 2 added, section 3 is revised, 3 references are added
dc.identifierhttps://arxiv.org/abs/0802.4349
dc.identifierhttp://arxiv.org/abs/0802.4349
dc.identifierGen.Rel.Grav.40:2515-2532,2008
dc.identifierdoi:10.1007/s10714-008-0635-3
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/211122
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleParticle Motion and Electromagnetic Fields of Rotating Compact Gravitating Objects with Gravitomagnetic Charge
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