Perturbation Method for Classical Spinning Particle Motion: I. Kerr Space-Time
arXiv:0808.3005 · doi:10.1103/PhysRevD.78.104028
Abstract
This paper presents an analytic perturbation approach to the dynamics of a classical spinning particle, according to the Mathisson-Papapetrou-Dixon (MPD) equations of motion, with a direct application to circular motion around a Kerr black hole. The formalism is established in terms of 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. Explicit expressions are determined for the case of circular motion near the event horizon a Kerr black hole, where the mass and spin shift contributions are dependent on the initial conditions of the particle's spin orientation. A preliminary analysis of the stability properties of the orbital motion in the Kerr background due to spin-curvature interactions is explored and briefly discussed.
23 pages; REVTeX file; 9 figures; Accepted for publication in Phys. Rev. D
References in corpus (12)
- Gravitational waves from a spinning particle in circular orbits around a rotating black hole
- Dynamics of spinning test particles in Kerr spacetime
- Innermost Stable Circular Orbit of a Spinning Particle in Kerr Spacetime
- A survey of spinning test particle orbits in Kerr spacetime
- Dynamics of Extended Spinning Masses in a Gravitational Field
- Relativistic Motion of Spinning Particles in a Gravitational Field
- Signature of chaos in gravitational waves from a spinning particle
- Tidal Dynamics in Kerr Spacetime
- On the motion of spinning test particles in plane gravitational waves
- Scattering of Spinning Test Particles by Plane Gravitational and Electromagnetic Waves
- Perturbation Method for Classical Spinning Particle Motion: II. Vaidya Space-Time
- An Analytic Perturbation Approach for Classical Spinning Particle Dynamics
Cited by in corpus (14)
- Spin dynamics in gravitational fields of rotating bodies and the equivalence principle
- Motion of spinning test bodies in Kerr spacetime
- Hamilton-Jacobi equation for spinning particles near black holes
- Motion of charged and spinning particle influenced by dark matter field surrounding a charged dyonic black hole
- Bounds on spinning particles in their innermost stable circular orbits around rotating braneworld black hole
- Mathisson-Papapetrou-Dixon equations in the Schwarzschild and Kerr backgrounds
- Fast Spinning Pulsars as Probes of Massive Black Holes' Gravity
- Highly relativistic spinning particle in the Schwarzschild field: Circular and other orbits
- Highly relativistic spinning particle starting near in a Kerr field
- Stability of circular orbits of spinning particles in Schwarzschild-like space-times
- Complex orbital dynamics of a double neutron star system revolving around a massive black hole
- Perturbation Method for Classical Spinning Particle Motion: II. Vaidya Space-Time
- Precisely computing bound orbits of spinning bodies around black holes I: General framework and results for nearly equatorial orbits
- Spinning test particles in the spacetime of a global monopole