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.

引用

页数：17

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