Gyroscope on polar orbit in the Kerr field

DOI10.1023/A:1010231810078zbMath0890.70004OpenAlexW99879581WikidataQ57666478 ScholiaQ57666478MaRDI QIDQ1364924

Oldřich Semerák

Publication date: 1 July 1998

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1023/a:1010231810078

zbMATH Keywords

black holesbackward Thomas precessionforward geodetic effectphoton geodesic spherical polar orbitzero-angular-momentum spherical polar orbit

Mathematics Subject Classification ID

Relativistic dynamics for problems in Hamiltonian and Lagrangian mechanics (70H40) Motion of the gyroscope (70E05)

Related Items (3)

Gyroscopic precession in the vicinity of a static blackhole's event horizon ⋮ Rotospheres in stationary axisymmetric spacetimes ⋮ Gyroscopic precession and inertial forces in axially symmetric stationary spacetimes

Cites Work

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• Rotating coordinates as tools for calculating circular geodesics and gyroscopic precession
• On calculation of magnetic-type gravitation and experiments
• Polar orbits in the Kerr space-time
• Physics of black holes. Transl. from the Russian by V. I. Kisin and E. M. Yankovsky
• Stationary frames in the Kerr field
• On the occurrence of rotospheres in the Kerr field
• Optical reference geometry for stationary and axially symmetric spacetimes
• Gyroscopic precession and inertial forces in the Kerr - Newman spacetime
• What forces act in relativistic gyroscope precession?

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