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.
โฆ LIBER โฆ
Three-dimensional cosmological gravity: Dynamics of constant curvature
โ Scribed by S Deser; R Jackiw
- Publisher
- Elsevier Science
- Year
- 1984
- Tongue
- English
- Weight
- 637 KB
- Volume
- 153
- Category
- Article
- ISSN
- 0003-4916
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