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Three-dimensional cosmological gravity: Dynamics of constant curvature

โœ 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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๐Ÿ“œ SIMILAR VOLUMES


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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.

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