arXiv · 1007.1961
From accelerating and Poincaré coordinates to black holes in spacelike warped AdS$_3$, and back
Abstract
We first review spacelike stretched warped AdS$_3$ and we describe its black hole quotients by using accelerating and Poincaré coordinates. We then describe the maximal analytic extension of the black holes and present their causal diagrams. Finally, we calculate spacetime limits of the black hole phase space $(T_R,T_L)$. This is done by requiring that the identification vector $\partial_θ$ has a finite non-zero limit. The limits we obtain are the self-dual solution in accelerating or Poincaré coordinates, depending respectively on whether the limiting spacetimes are non-extremal or extremal, and warped AdS with a periodic proper time identification.
Explore related subjects
Keep this discovery
Frederic Jugeau, George Moutsopoulos, Patricia Ritter. 2010-12-11. From accelerating and Poincaré coordinates to black holes in spacelike warped AdS$_3$, and back. https://doi.org/10.1088/0264-9381%2F28%2F3%2F035001
Cite the original work for its findings. Save a collection to share your selection of sources.