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2013 | OriginalPaper | Chapter

The C-Boundary Construction of SpaceTimes: Application to Stationary Kerr SpaceTime

Authors : J. L. Flores, J. Herrera

Published in: Recent Trends in Lorentzian Geometry

Publisher: Springer New York

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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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Footnotes
1
We will use typical background and terminology in Lorentzian geometry as in [2, 15, 16].
 
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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Metadata
Title
The C-Boundary Construction of SpaceTimes: Application to Stationary Kerr SpaceTime
Authors
J. L. Flores
J. Herrera
Copyright Year
2013
Publisher
Springer New York
DOI
https://doi.org/10.1007/978-1-4614-4897-6_11

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