2003/07/31 by Z. Stuchlik, P. Slany · 2 citations
Physics and Astronomy · #gr-qc
paper · pdf · doi:10.1103/physrevd.69.064001
published as Phys.Rev. D69 (2004) 064001 · 24 pages, 19 figures, REVTeX 4
arxiv created 2004/04/14 · arxiv updated 2009/12/01
Equatorial motion of test particles in the Kerr-de Sitter spacetimes is considered. Circular orbits are determined, their properties are discussed for both the black-hole and naked-singularity spacetimes, and their relevance for thin accretion discs is established.