Journal
GENERAL RELATIVITY AND GRAVITATION
Volume 41, Issue 11, Pages 2579-2586Publisher
SPRINGER/PLENUM PUBLISHERS
DOI: 10.1007/s10714-009-0781-2
Keywords
Painleve-Gullstrand coordinates; Kerr solution
Funding
- Fundacao para a Ciencia e a Tecnologia [POCI 2010/FEDER]
- [POCI/MAT/58549/2004]
- Fundação para a Ciência e a Tecnologia [POCI/MAT/58549/2004] Funding Source: FCT
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We construct a coordinate system for the Kerr solution, based on the zero angular momentum observers dropped from infinity, which generalizes the Painlev,-Gullstrand coordinate system for the Schwarzschild solution. The Kerr metric can then be interpreted as describing space flowing on a (curved) Riemannian 3-manifold. The stationary limit arises as the set of points on this manifold where the speed of the flow equals the speed of light, and the horizons as the set of points where the radial speed equals the speed of light. A deeper analysis of what is meant by the flow of space reveals that the acceleration of free-falling objects is generally not in the direction of this flow. Finally, we compare the new coordinate system with the closely related Doran coordinate system.
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