Stellar Equilibrium in 2+1 Dimensions
Preprint
- 13 November 1994
Abstract
The hydrostatic equilibrium of a $2+1$ dimensional perfect fluid star in asymptotically anti-de Sitter space is discussed. The interior geometry matches the exterior $2+1$ black-hole solution. An upper mass limit is found, analogous to Buchdahl's theorem in 3+1, and the possibility of collapse is discussed. The case of a uniform matter density is solved exactly and a new interior solution is presented.
Keywords
All Related Versions
- Version 1, 1994-11-13, ArXiv
- Published version: Classical and Quantum Gravity, 12 (4), 975.
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