Physical effects in the Vaidya–Einstein–Kerr spacetime

DOI10.1088/0264-9381/20/24/002zbMath1047.83023OpenAlexW1996260218MaRDI QIDQ4453750

C. V. Vishveshwara, B. S. Ramachandra

Publication date: 7 March 2004

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

Full work available at URL: https://doi.org/10.1088/0264-9381/20/24/002

zbMATH Keywords

rotating black holescircular geodesicsgyroscopic precissionVaidya-Einstein-Kerr space-time

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Black holes (83C57) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Astrophysical cosmology (85A40)

Related Items (3)

The Carter constant and Petrov classification of the Vaidya-Einstein-Kerr spacetime ⋮ Gyroscopic precession in the vicinity of a static blackhole's event horizon ⋮ Kerr black hole in the background of the Einstein universe

This page was built for publication: Physical effects in the Vaidya–Einstein–Kerr spacetime