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Published on: November 15, 2013
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Characterizations of Kerr-de Sitter in arbitrary dimension from null infinity
M Mars1, C Peón-Nieto1,2
1Universidad de Salamanca, Salamanca, Spain.
Summary
Researchers characterized higher-dimensional Kerr-de Sitter metrics by analyzing their behavior at future null infinity. This approach defines a larger Kerr-de Sitter-like class with specific asymptotic properties.
Area of Science:
- * General Relativity
- * Mathematical Physics
Background:
- * Kerr and Kerr-de Sitter metrics possess unique local geometric properties in four dimensions.
- * Generalizations to higher dimensions lack this local characterization, necessitating alternative analysis methods.
- * Understanding behavior at future null infinity offers a viable approach for characterizing these higher-dimensional metrics.
Purpose of the Study:
- * To generalize the characterization of Kerr-de Sitter metrics to higher dimensions.
- * To explore the asymptotic properties of higher-dimensional spacetimes using established formalisms.
- * To define and characterize the broader Kerr-de Sitter-like class of metrics.
Main Methods:
- * Review of Friedrich's and Fefferman-Graham formalisms for asymptotic initial value problems.
- * Analysis of (anti-)de Sitter-vacuum spacetimes in arbitrary dimensions.
- * Study of geometric identification, conformal equivalence of data, and Killing initial data.
- * Investigation of conformal equivalence of boundary conformal Killing vectors (CKV).
Main Results:
- * Characterization of Kerr-de Sitter metrics via conformal flatness and a canonical TT tensor constructed from CKV at null infinity.
- * Definition of the Kerr-de Sitter-like class, encompassing metrics with arbitrary CKV.
- * Explicit construction of these metrics as limits or analytic extensions of Kerr-de Sitter.
- * Identification of Kerr-Schild property and specific falloff conditions for this class.
- * In five dimensions, correspondence to algebraically special metrics with non-degenerate optical matrices.
Conclusions:
- * The asymptotic data at future null infinity provides a robust method for characterizing higher-dimensional Kerr-de Sitter-like spacetimes.
- * The defined Kerr-de Sitter-like class offers a comprehensive framework for studying these complex metrics.
- * These findings contribute to understanding the interplay of asymptotics, conformal methods, and analysis in general relativity.
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