Black Hole Entropy from Entangled Quantum Reference Frames

@misc{varrin2026black,
  title = {{Black Hole Entropy from Entangled Quantum Reference Frames}},
  author = {Ludovic Varrin},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.37750},
  eprint = {2610.37750},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.37750},
}

TY  - UNPB
TI  - Black Hole Entropy from Entangled Quantum Reference Frames
AU  - Ludovic Varrin
PY  - 2026
DA  - 2026/10/27
PB  - arXiv
DO  - 10.48550/arxiv.2610.37750
UR  - https://arxiv.org/abs/2610.37750
AB  - In the extended phase space of Donnelly and Freidel, the edge modes of a Schwarzschild black hole are dynamical reference frames whose phase space is the cotangent bundle of SL(2,ℝ). Gluing the two exterior regions at the bifurcation point leaves a single canonical pair. Within the extended phase space, this pair can be described either by Kuchař's mass and difference of asymptotic times or by the area and the relative rapidity of the two frames, which are two gauge choices of the same system. The latter is the pair of Carlip and Teitelboim, and the relative rapidity is the time shift of the crossed product construction. We quantize the frames in this gauge and construct the gravitational entangling product of the two exteriors. Requiring the frames to be causal restricts them to the semigroup SL^+(2,ℝ), whose Plancherel measure yields the Bekenstein--Hawking entropy as the entanglement entropy between the two exteriors, together with a logarithmic correction, both independent of the ultraviolet cutoff.
ER  -