Holography in asymptotically flat spacetimes and the BMS group

DOI10.1088/0264-9381/21/23/022zbMath1065.83018arXivhep-th/0312186OpenAlexW2398723015MaRDI QIDQ4659410

Giovanni Arcioni, Claudio Dappiaggi

Publication date: 21 March 2005

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/hep-th/0312186

Mathematics Subject Classification ID

Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (13)

Flat holography and Carrollian fluids ⋮ Universal corner symmetry and the orbit method for gravity ⋮ Carrollian conformal scalar as flat-space singleton ⋮ Enhanced asymptotic \(BMS_{3}\) algebra of the flat spacetime solutions of generalized minimal massive gravity ⋮ Foliation-based quantization and black hole information ⋮ Quasi-local holographic dualities in non-perturbative 3d quantum gravity. I: Convergence of multiple approaches and examples of Ponzano-Regge statistical duals ⋮ Aspects of the BMS/CFT correspondence ⋮ Quantum out-states holographically induced by asymptotic flatness: invariance under spacetime symmetries, energy positivity and Hadamard property ⋮ Double-soft graviton amplitudes and the extended BMS charge algebra ⋮ Asymptotic structure of Einstein-Maxwell-dilaton theory and its five dimensional origin ⋮ BMS₃ mechanics and the black hole interior ⋮ RIGOROUS STEPS TOWARDS HOLOGRAPHY IN ASYMPTOTICALLY FLAT SPACETIMES ⋮ ON THE LAGRANGIAN AND HAMILTONIAN FORMULATION OF A SCALAR FREE FIELD THEORY AT NULL INFINITY

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