Gyroscope precession along unbound equatorial plane orbits around a Kerr black hole

被引：8
作者：
Bini, Donato [1 ]
Geralico, Andrea [2 ]
Jantzen, Robert T. [3 ]
机构：
[1] CNR, Ist Applicaz Calcolo M Picone, I-00185 Rome, Italy
[2] INAF, Astrophys Observ Torino, I-10025 Pino Torinese, TO, Italy
[3] Villanova Univ, Dept Math & Stat, Villanova, PA 19085 USA
来源：
PHYSICAL REVIEW D | 2016年 / 94卷 / 12期
关键词：
STATIONARY AXISYMMETRICAL SPACETIMES; FRENET-SERRET DESCRIPTION; SPINNING TEST PARTICLES; THOMAS PRECESSION; CIRCULAR ORBITS; SCHWARZSCHILD SPACETIME; GENERAL-RELATIVITY; GRAVITATIONAL THEORY; CENTRIFUGAL FORCES; WIGNER ROTATION;
D O I：
10.1103/PhysRevD.94.124002
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The precession of a test gyroscope along unbound equatorial plane geodesic orbits around a Kerr black hole is analyzed with respect to a static reference frame whose axes point towards the "fixed stars." The accumulated precession angle after a complete scattering process is evaluated and compared with the corresponding change in the orbital angle. Limiting results for the nonrotating Schwarzschild black hole case are also discussed.
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页数：17
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