Strong gravity Lense–Thirring precession in Kerr and Kerr–Taub–NUT spacetimes

DOI10.1088/0264-9381/31/7/075006zbMath1291.83038arXiv1304.6936OpenAlexW3104473226MaRDI QIDQ5416469

Chrachur Chakraborty, Parthasarathi Majumdar

Publication date: 20 May 2014

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1304.6936

zbMATH Keywords

precessionstrongTaub-NUT spacetimeLense-ThirringKerr-Taub-NUT (Newman-Unti-Tamburino)

Mathematics Subject Classification ID

Black holes (83C57) Galactic and stellar dynamics (85A05) Equations of motion in general relativity and gravitational theory (83C10)

Related Items (11)

Center of mass energy of the collision for two general geodesic particles around a Kerr-Newman-Taub-NUT black hole ⋮ Inertial Frame Dragging in an Acoustic Analogue Spacetime ⋮ Gyroscopic precession in the vicinity of a static blackhole's event horizon ⋮ Exact massive and massless scalar quasibound states around a charged Lense-Thirring black hole ⋮ Circular orbits in the Taub–NUT and massless Taub–NUT spacetime ⋮ Generalized planar black holes and the holography of hydrodynamic shear ⋮ Strong cosmic censorship conjecture with NUT charge and conformal coupling ⋮ Distinguishing between Kerr and rotating JNW space-times via frame dragging and tidal effects ⋮ Rotating normal and phantom Einstein–Maxwell–dilaton black holes: Geodesic analysis ⋮ Circular orbits in Kerr-Taub-NUT spacetime and their implications for accreting black holes and naked singularities ⋮ Behavior of a test gyroscope moving towards a rotating traversable wormhole

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