The DOI matches its Crossref record; 25 of the 25 references it cites were found in a registry or an index.
Asymptotic structure of symmetry-reduced general relativity
Open accessAbstract
Gravitational waves with a space-translation Killing field are considered. Because of the symmetry, the four-dimensional Einstein vacuum equations are equivalent to the three-dimensional Einstein equations with certain matter sources. This interplay between four- and three-dimensional general relativity can be exploited effectively to analyze issues pertaining to four dimensions in terms of the three-dimensional structures. An example is provided by the asymptotic structure at null infinity: While these space-times fail to be asymptotically flat in four dimensions, they can admit a regular completion at null infinity in three dimensions. This completion is used to analyze the asymptotic symmetries, introduce the analogue of the four-dimensional Bondi energy momentum, and write down a flux formula. The analysis is also of interest from a purely three-dimensional perspective because it pertains to a diffeomorphism-invariant three-dimensional field theory with local degrees of freedom, i.e., to a midisuperspace. Furthermore, because of certain peculiarities of three dimensions, the description of null infinity has a number of features that are quite surprising because they do not arise in the Bondi-Penrose description in four dimensions.
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Cited by
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Metadata
- Authors
- Ashtekar, A., Bičák, J., & Schmidt, B. G.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 1997-01-15
- Volume
- 55
- Issue
- 2
- Pages
- 669-686
- ISSN
- 0556-2821 (ISSN-L)
- 1089-4918
- OpenAlex
- W2050984773
- Cited by
- 255
- References
- 25
- FWCI
- 5.59
- Type
- journal article
- Language
- en
- Open access
- green
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