Gyroscope precession along bound equatorial plane orbits around a Kerr black hole
arXiv:1607.08427 · doi:10.1103/PhysRevD.94.064066
Abstract
The precession of a test gyroscope along stable bound equatorial plane orbits around a Kerr black hole is analyzed and the precession angular velocity of the gyro's parallel transported spin vector and the increment in precession angle after one orbital period is evaluated. The parallel transported Marck frame which enters this discussion is shown to have an elegant geometrical explanation in terms of the electric and magnetic parts of the Killing-Yano 2-form and a Wigner rotation effect.
16 pages; revtex macros; 3 eps figures
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Cited by in corpus (5)
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- Spin-orbit precession for eccentric black hole binaries at first order in the mass ratio
- Gyroscope precession along unbound equatorial plane orbits around a Kerr black hole
- High-order post-Newtonian expansion of the generalized redshift invariant for eccentric-orbit, equatorial extreme-mass-ratio inspirals with a spinning primary
- The Orbital Lense-Thirring Precession in a Strong Field