Dynamics of Extended Spinning Masses in a Gravitational Field

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dc.creatorMashhoon, Bahram
dc.creatorSingh, Dinesh
dc.date2006-08-13
dc.date2006-11-30
dc.date.accessioned2026-07-07T12:16:28Z
dc.date.available2026-07-07T12:16:28Z
dc.descriptionWe develop a first-order approximation method for the influence of spin on the motion of extended spinning test masses in a gravitational field. This approach is illustrated for approximately circular equatorial motion in the exterior Kerr spacetime. In this case, the analytic results for the first-order approximation are compared to the numerical integration of the exact system and the limitations of the first-order results are pointed out. Furthermore, we employ our analytic results to illustrate the gravitomagnetic clock effect for spinning particles.
dc.description16 pages, 3 figures; v2: 15 pages, 3 figures, improved version to appear in Phys. Rev. D
dc.identifierhttps://arxiv.org/abs/astro-ph/0608278
dc.identifierhttp://arxiv.org/abs/astro-ph/0608278
dc.identifierPhys.Rev.D74:124006,2006
dc.identifierdoi:10.1103/PhysRevD.74.124006
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/211810
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleDynamics of Extended Spinning Masses in a Gravitational Field
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