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Flat limit of three dimensional asymptotically anti–de Sitter spacetimes
Open accessAbstract
In order to get a better understanding of holographic properties of gravitational theories with a vanishing cosmological constant, we analyze in detail the relation between asymptotically anti-de Sitter and asymptotically flat spacetimes in three dimensions. This relation is somewhat subtle because the limit of vanishing cosmological constant cannot be naively taken in standard Fefferman-Graham coordinates. After reformulating the standard anti-de Sitter results in Robinson-Trautman coordinates, a suitably modified Penrose limit is shown to connect both asymptotic regimes.
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Cites
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Metadata
- Authors
- Barnich, G., Gomberoff, A., & González, H. A.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 2012-07-10
- Volume
- 86
- Issue
- 2
- ISSN
- 0556-2821 (ISSN-L)
- 1550-7998
- 1550-2368
- OpenAlex
- W2025277621
- Cited by
- 269
- References
- 50
- FWCI
- 6.00
- Type
- journal article
- Language
- en
- Open access
- green
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- Barnich, G., Gomberoff, A., & González, H. A. (2012). Flat limit of three dimensional asymptotically anti–de Sitter spacetimes. Physical Review D. https://doi.org/10.1103/physrevd.86.024020
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