Plane waves and spacelike infinity

Abstract

In an earlier paper, we showed that the causal boundary of any homogeneous plane wave satisfying the null convergence condition consists of a single null curve. In Einstein-Hilbert gravity, this would include any homogeneous plane wave satisfying the weak null energy condition. For conformally flat plane waves such as the Penrose limit of $Ad{S}_5\times S^5$, all spacelike curves that reach infinity also end on this boundary and the completion is Hausdorff. However, the more generic case (including, e.g., the Penrose limits of $Ad{S}_4\times S^7$ and $Ad{S}_7\times S^4$) is more complicated. In one natural topology, not all spacelike curves have limit points in the causal completion, indicating the need to introduce additional points at `spacelike infinity'--the endpoints of spacelike curves. We classify the distinct ways in which spacelike curves can approach infinity, finding a {\it two}-dimensional set of distinct limits. The dimensionality of the set of points at spacelike infinity is not, however, fixed from this argument. In an alternative topology, the causal completion is already compact, but the completion is non-Hausdorff.

18 pages, 3 figures, minor changes

References in corpus (4)

• On lightcone string field theory from Super Yang-Mills and holography
• A new recipe for causal completions
• On the Singularity Structure and Stability of Plane Waves
• Penrose Limits of RG Fixed Points and PP-Waves with Background Fluxes

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