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arXiv · 1006.3099

Non-Einstein geometries in Chiral Gravity

Geoffrey Compère·Sophie de Buyl·Stéphane Detournay
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Abstract

We analyze the asymptotic solutions of Chiral Gravity (Topologically Massive Gravity at μl = 1 with Brown-Henneaux boundary conditions) focusing on non-Einstein metrics. A class of such solutions admits curvature singularities in the interior which are reflected as singularities or infinite bulk energy of the corresponding linear solutions. A non-linear solution is found exactly. The back-reaction induces a repulsion of geodesics and a shielding of the singularity by an event horizon but also introduces closed timelike curves.

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Geoffrey Compère, Sophie de Buyl, Stéphane Detournay. 2010-08-25. Non-Einstein geometries in Chiral Gravity. https://doi.org/10.1007/jhep10(2010)042

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