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Stationary axisymmetric solutions of three-dimensional Einstein gravity

✍ Scribed by S. Deser; B. Laurent


Publisher
Springer US
Year
1986
Tongue
English
Weight
564 KB
Volume
18
Category
Article
ISSN
0001-7701

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Three-dimensional Einstein gravity: Dyna
✍ S Deser; R Jackiw; G 't Hooft πŸ“‚ Article πŸ“… 1984 πŸ› Elsevier Science 🌐 English βš– 828 KB

In three spacetime dimensions, the Einstein equations imply that source-free regions are flat. Localized sources can therefore only affect geometry globally rather than locally. Some of these effects, especially those generated by mass and angular momentum are discussed.