Abstract
The aim of this chapter is twofold. First, we review several results about the c-boundary of space-times and other boundaries in differential geometry, completing some points which were suggested in the original works. Second, we are going to apply these results to provide a precise description of the c-boundary of the stationary part of (slow rotating) Kerr space time.
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Notes
- 1.
- 2.
This section is the development of a seminal idea by Prof. Miguel Sánchez (see also [17]).
- 3.
In this proposition, by the term “Busemann completion,” we must understand the usual Busemann completion up to its asymptotic region,that is, those points of the Busemann boundary associated to curves with diverging radial component.
- 4.
For simplicity, the elements \([x] \in [-6, 6]/R\) will be denoted by x.
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Acknowledgements
The authors acknowledge Prof. Miguel Sánchez the valuable supervision of this work, and the comments by the referee. The authors are partially supported by the Spanish MICINN Grant MTM2010-18099 and Regional J. Andalucía Grant P09-FQM-4496, both with FEDER funds.
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Flores, J.L., Herrera, J. (2012). The C-Boundary Construction of SpaceTimes: Application to Stationary Kerr SpaceTime. In: Sánchez, M., Ortega, M., Romero, A. (eds) Recent Trends in Lorentzian Geometry. Springer Proceedings in Mathematics & Statistics, vol 26. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-4897-6_11
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