Vacuum energy in asymptotically flat \(2+1\) gravity
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Publication:1634921
DOI10.1016/j.physletb.2017.02.006zbMath1404.83077arXiv1610.06101OpenAlexW2535446549MaRDI QIDQ1634921
Rodrigo Olea, Olivera Miskovic, Debraj Roy
Publication date: 18 December 2018
Published in: Physics Letters. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1610.06101
Analogues of general relativity in lower dimensions (83C80) Yang-Mills and other gauge theories in mechanics of particles and systems (70S15)
Related Items (3)
Generalized Maxwellian exotic Bargmann gravity theory in three spacetime dimensions ⋮ Asymptotic symmetries of three-dimensional Chern-Simons gravity for the Maxwell algebra ⋮ On stabilization of Maxwell-BMS algebra
Cites Work
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- Role of surface integrals in the Hamiltonian formulation of general relativity
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- Entropy of three-dimensional asymptotically flat cosmological solutions
- New supergravities with central charges and Killing spinors in \(2+1\) dimensions
- The dynamical structure of higher dimensional Chern-Simons theory
- Aspects of the BMS/CFT correspondence
- CHERN–SIMONS THEORIES WITH SUPERSYMMETRIES IN THREE DIMENSIONS
- Classical central extension for asymptotic symmetries at null infinity in three spacetime dimensions
- Aspects of flat/CCFT correspondence
- The asymptotic dynamics of three-dimensional Einstein gravity with a negative cosmological constant
- A Neumann boundary term for gravity
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