Vacuum energy in asymptotically flat 2+1 gravity
arXiv:1610.06101 · doi:10.1016/j.physletb.2017.02.006
Abstract
We compute the vacuum energy of three-dimensional asymptotically flat space based on a Chern-Simons formulation for the Poincare group. The equivalent action is nothing but the Einstein-Hilbert term in the bulk plus half of the Gibbons-Hawking term at the boundary. The derivation is based on the evaluation of the Noether charges in the vacuum. We obtain that the vacuum energy of this space has the same value as the one of the asymptotically flat limit of three-dimensional anti-de Sitter space.
15 pages, no figures; introduction extended, references added
References in corpus (6)
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- Flat-Space Chiral Gravity
- On boundary conditions in three-dimensional AdS gravity
- Aspects of Flat/CCFT Correspondence
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- The non-zero energy of 2+1 Minkowski space