General description of Dirac spin-rotation effect with relativistic factor

dc.creatorZhang, C. M.
dc.date2007-01-07
dc.date.accessioned2026-07-07T10:22:04Z
dc.date.available2026-07-07T10:22:04Z
dc.descriptionThe Mashhoon rotation-spin coupling is studied by means of the parallelism description of general relativity. The relativistic rotational tetrad is exploited, which results in the Minkowski metric, and the torsion axial-vector and Dirac spin coupling will give the Mashhoon rotation-spin term. For the high speed rotating cases, the tangent velocity constructed by the angular velocity $\Ome$ multiplying the distance r may exceed over the speed of light c, i.e., $\Ome r \ge c$, which will make the relativistic factor $γ$ infinity or imaginary. In order to avoid this "meaningless" difficulty occurred in $γ$ factor, we choose to make the rotation nonuniform and position-dependent in a particular way, and then we find that the new rotation-spin coupling energy expression is consistent with the previous results in the low speed limit.
dc.description8 pages, accepted by IJMPD 2007
dc.identifierhttps://arxiv.org/abs/gr-qc/0701044
dc.identifierhttp://arxiv.org/abs/gr-qc/0701044
dc.identifierInt.J.Mod.Phys.D16:737-744,2007
dc.identifierdoi:10.1142/S0218271807009875
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/175387
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGeneral description of Dirac spin-rotation effect with relativistic factor
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