Non-trivial, static, geodesically complete, vacuum space-times with a negative cosmological constant

By Michael T. Anderson, Piotr T. Chruściel, E. Delay. 2002

192 citations recorded by the source corpus.

We construct a large class of new singularity-free static lorentzian four-dimensional solutions of the vacuum Einstein equations with a negative cosmological constant. The new families of metrics contain space-times with, or without, black hole regions. Two uniqueness results are also established.

Subfields: Applied Mathematics, Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/92d40b06bae655cbd882ffa87931bc2fde958bfd

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Applied Mathematics

1. Jorge E Santos
2. Ó. J. Dias
3. G. Horowitz

In Astronomy and Astrophysics

1. Jorge E Santos
2. Ó. J. Dias
3. G. Horowitz
4. Benson Way
5. V. Cardoso
6. Paolo Pani
7. S. Hartnoll
8. Aristomenis Donos

In Nuclear and High Energy Physics

1. Jorge E Santos
2. Ó. J. Dias
3. G. Horowitz
4. Benson Way
5. Aristomenis Donos
6. V. Cardoso
7. Blaise Goutéraux
8. J. Gauntlett

Citations in the corpus

• Black holes with only one Killing field (2011, methodology): “1 Another way to construct asymptotically AdS black holes with only one Killing eld is to modify the boundary conditions at innity so that the boundary metric is not conformal to a round sphere cross time [ 5 ].”