Spontaneously broken asymptotic symmetries and an effective action for horizon dynamics

DOI10.1007/JHEP02(2017)052zbMath1377.83041arXiv1611.10214MaRDI QIDQ1692810

Christopher Eling

Publication date: 10 January 2018

Published in: Journal of High Energy Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1611.10214

zbMATH Keywords

black holes2D gravityspace-time symmetriesRaychaudhuri equationDilaton gravity

Mathematics Subject Classification ID

Black holes (83C57) Symmetry breaking in quantum theory (81R40) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Analogues of general relativity in lower dimensions (83C80) Equations of motion in general relativity and gravitational theory (83C10)

Related Items (6)

Are non-vacuum states much relevant for retrieving shock wave memory of spacetime? ⋮ Near-horizon BMS symmetries as fluid symmetries ⋮ Null boundary terms for Lanczos-Lovelock gravity ⋮ Asymptotic symmetries of three dimensional gravity and the membrane paradigm ⋮ BMS₃invariant fluid dynamics at null infinity ⋮ BMS Goldstone modes near the horizon of a Kerr black hole are thermal

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