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- W2317695989 abstract "An analytic perturbation approach to the dynamics of a classical spinning particle is presented, according to the Mathisson-Papapetrou-Dixon (MPD) equations of motion, with application to circular motion around astrophysical black holes. The formalism is based on a power series expansion with respect to the particle’s spin magnitude, where the particle’s kinematic and dynamical degrees are expressed in a completely general form that can be constructed to infinite order in the expansion parameter. It is further shown that the particle’s squared mass and spin magnitude can shift due to a classical analogue of radiative corrections that arise from spin-curvature coupling." @default.
- W2317695989 created "2016-06-24" @default.
- W2317695989 creator A5068478097 @default.
- W2317695989 date "2012-02-01" @default.
- W2317695989 modified "2023-09-28" @default.
- W2317695989 title "CLASSICAL SPINNING PARTICLE INTERACTIONS IN BLACK HOLE SPACE-TIME BACKGROUNDS" @default.
- W2317695989 doi "https://doi.org/10.1142/9789814374552_0403" @default.
- W2317695989 hasPublicationYear "2012" @default.
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