Formation of Black Holes in Topologically Massive Gravity
arXiv:1108.3579 · doi:10.1103/PhysRevD.87.024019
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 horizon
Improved presentation. Extended discussion of linear stability and regularity of the metric. Added references
References in corpus (5)
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- Asymptotically anti-de Sitter spacetimes in topologically massive gravity
- Asymptotically warped anti-de Sitter spacetimes in topologically massive gravity
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Cited by in corpus (5)
- Holographic applications of logarithmic conformal field theories
- On complexity growth in massive gravity theories, the effects of chirality and more
- Chiral Massive News: Null Boundary Symmetries in Topologically Massive Gravity
- Dynamical Black Holes in 2+1 Dimensions
- Null Surface Thermodynamics in Topologically Massive Gravity