FORCES IN KERR SPACE–TIMES WITH A REPULSIVE COSMOLOGICAL CONSTANT
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Publication:3422255
DOI10.1142/S0217751X06032435zbMath1133.83311arXivgr-qc/0611152MaRDI QIDQ3422255
Publication date: 9 February 2007
Published in: International Journal of Modern Physics A (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/gr-qc/0611152
Black holes (83C57) Space-time singularities, cosmic censorship, etc. (83C75) Exact solutions to problems in general relativity and gravitational theory (83C15) Equations of motion in general relativity and gravitational theory (83C10)
Related Items (3)
Charged fluids encircling compact objects: force representations and conformal geometries ⋮ PSEUDO-NEWTONIAN GRAVITATIONAL POTENTIAL FOR SCHWARZSCHILD–DE SITTER SPACE–TIMES ⋮ RELATIVISTIC DYNAMICS WITH COSMOLOGICAL CONSTANT: CIRCULAR GEODESIC MOTION OF TEST PARTICLES
Cites Work
- Optical reference geometry for stationary and static dynamics
- Optical space of the Reissner-Nordström solutions
- Curving Newtonian space
- Gravitational waves from ultracompact stars: the optical geometry view of trapped modes
- Covariant definition of inertial forces
- Optical reference geometry of Kerr-Newman spacetimes
- Photon capture cones and embedding diagrams of the Ernst spacetime
- Optical reference geometry for stationary and axially symmetric spacetimes
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