Dirac Spin Precession in Kerr Spacetime by the parallelism description

dc.creatorZhang, C. M.
dc.date2004-05-28
dc.date.accessioned2026-07-07T07:39:04Z
dc.date.available2026-07-07T07:39:04Z
dc.descriptionIn the framework of parallelism general relativity (PGR), the Dirac particle spin precession in the rotational gravitational field is studied. In terms of the equivalent tetrad of Kerr frame, we investigate the torsion axial-vector spin coupling in PGR. In the case of the weak field and slow rotation approximation, we obtain that the torsion axial-vector has the dipole-like structure, but different from the gravitomagnetic field, which indicates that the choice of the Kerr tetrad will influence on the physics interpretation of the axial-vector spin coupling.
dc.description6 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/0405138
dc.identifierhttp://arxiv.org/abs/gr-qc/0405138
dc.identifierCommun.Theor.Phys. 44 (2005) 279-286
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/121313
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleDirac Spin Precession in Kerr Spacetime by the parallelism description
dc.typetext

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