One loop partition function of three-dimensional flat gravity
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Publication:2635319
DOI10.1007/JHEP04(2015)178zbMath1388.83086arXiv1502.06185OpenAlexW3098995211MaRDI QIDQ2635319
Glenn Barnich, Blagoje Oblak, Alexander Maloney, Hernán A. González
Publication date: 31 May 2018
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1502.06185
topological field theoriesclassical theories of gravityconformal and W symmetryspace-time symmetries
Quantum field theory on curved space or space-time backgrounds (81T20) Quantization of the gravitational field (83C45)
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Cites Work
- Quantum gravity partition functions in three dimensions
- The heat kernel on \(\text{AdS}_3\) and its applications
- Characters of the BMS group in three dimensions
- Central charges in the canonical realization of asymptotic symmetries: An example from three dimensional gravity
- Two dimensional gauge theories revisited
- Role of surface integrals in the Hamiltonian formulation of general relativity
- Notes on the BMS group in three dimensions. II: Coadjoint representation
- Entropy of three-dimensional asymptotically flat cosmological solutions
- TRANSITION AMPLITUDE IN (2+1)-DIMENSIONAL CHERN-SIMONS GRAVITY ON A TORUS
- Classical central extension for asymptotic symmetries at null infinity in three spacetime dimensions
- Time‐dependent orbifolds and string cosmology
- Black hole in three-dimensional spacetime
- Quantizing gravity with a cosmological constant
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