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Formation of Black Holes in Topologically Massive Gravity

Abstract

We present an exact solution in 3-dimensional topologically massive gravity with negative cosmological constant which dynamically interpolates between a past horizon and a chiral AdS pp-wave. Similarly, upon time reversal, one obtains an AdS pp-wave with a future event horizonComment: Improved presentation. Extended discussion of linear stability and regularity of the metric. Added reference

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