
TL;DR
This paper connects the microscopic degrees of freedom responsible for black hole entropy to phase space states distinguished by Hamiltonian surface charges, using a generalized Ryu-Takayanagi formula.
Contribution
It demonstrates that black hole microstates can be identified via Hamiltonian surface charges in diffeomorphism invariant theories, linking them to Wald entropy.
Findings
Black hole microstates correspond to phase space states distinguished by surface charges.
The generalized Ryu-Takayanagi formula relates these states to entanglement and entropy.
The approach uncovers black hole hair hidden in naive spacetime interpretations.
Abstract
Applications of the Ryu-Takayanagi formula to evaporating black holes are known to reproduce the Page curve, although leaving open the microscopic origin of the necessary black hole degrees of freedom responsible for the entanglement and microstates. Here, we fill this gap by utilizing a recently proven generalized Ryu-Takayanagi formula which keeps the contact to the theory's Hamiltonian phase space. Precisely, we show that in any diffeomorphism invariant field theory containing stationary black holes with bifurcate Killing horizons the phase space states distinguishable by their Hamiltonian surface charges over the bifurcation surface must provide the degrees of freedom responsible for the black hole's Wald entropy. This result is part of a larger program where measurable quantities of a quantum theory are expressed as weighted sums over paths in the theory's phase space. Suited…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
