Near-Horizon BMS Symmetry, Dimensional Reduction, and Black Hole Entropy
arXiv:1910.01762 · doi:10.1103/PhysRevD.101.046002
Abstract
In an earlier short paper [Phys.\ Rev.\ Lett.\ 120 (2018) 101301, arXiv:1702.04439], I argued that the horizon-preserving diffeomorphisms of a generic black hole are enhanced to a larger BMS symmetry, which is powerful enough to determine the Bekenstein-Hawking entropy. Here I provide details and extensions of that argument, including a loosening of horizon boundary conditions and a more thorough treatment of dimensional reduction and meaning of a "near-horizon symmetry."
28 pages; longer, more detailed (and extended) version of arXiv:1702.04439
References in corpus (7)
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- Notes on the BMS group in three dimensions: I. Induced representations
- Notes on the BMS group in three dimensions: II. Coadjoint representation
- Noether current from the surface term of gravitational action, Virasoro algebra and horizon entropy
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- Isolated Surfaces and Symmetries of Gravity
- Universal Corner Symmetry and the Orbit Method for Gravity
- Carroll covariant scalar fields in two dimensions
- A Rindler Road to Carrollian Worldsheets
- BMS Field Theories and Weyl Anomaly
- Entropy in Poincaré gauge theory: Kerr-AdS solution
- Near horizon gravitational charges
- Stress tensors of 3d Carroll CFTs
- Quadratic and cubic spherically symmetric black holes in the modified teleparallel equivalent of general relativity: Energy and thermodynamics
- BMS Mechanics and the Black Hole Interior
- Quantum Mechanics of a Spherically Symmetric Causal Diamond in Minkowski Spacetime
- A Schwarzian on the Stretched Horizon
- Gauge theories with non-trivial boundary conditions: Black holes
- Complexity growth of BTZ black hole in massive gravity with a null string
- On energy for accelerating observers in black hole spacetimes
- Counting Black Hole Microstates at Future Null Infinity
- A note on the action with the Schwarzian at the stretched horizon
- Hidden Symmetries in Gravity : Black holes and other minisuperspaces