Probing black hole entropy via entanglement

Shuxuan Ying

doi:10.1016/j.nuclphysb.2026.117377

paper

Probing black hole entropy via entanglement

arXiv:2505.08012 · doi:10.1016/j.nuclphysb.2026.117377

Abstract

In this paper, we develop a method to extract the Bekenstein-Hawking entropy of $D$ -dimensional black holes using the entanglement entropy of a lower-dimensional conformal field theory (CFT). This approach relies on two key observations. On the gravitational side, the near-horizon geometry of extremal black holes is AdS $_{2}$ , and the Bekenstein-Hawking entropy is entirely determined by this two-dimensional geometry. Moreover, the higher-dimensional spherical part of the black hole metric is absorbed into the $D$ -dimensional Newton's constant $G_{N}^{(D)}$ , which can be effectively reduced to a two-dimensional Newton's constant $G_{N}^{(2)}$ . On the field theory side, the entanglement entropy of two disconnected one-dimensional conformal quantum mechanics (CQM $_{1}$ ) can be calculated. According to the Ryu-Takayanagi (RT) prescription, this entanglement entropy computes the area of the minimal surface in the AdS $_{2}$ geometry. Since the near-horizon region of the black hole and the emergent spacetime derived from the entanglement entropy share the same Penrose diagram -- with both the black hole event horizon and the RT surface corresponding to specific points on this diagram -- the Bekenstein-Hawking entropy can be probed via entanglement entropy when these points coincide. This result explicitly demonstrates that the entanglement across the event horizon is the fundamental origin of the Bekenstein-Hawking entropy.

V1: 20 pages, 12 figures; V2: 22pages, 12 figures, references added, published version in Nucl. Phys. B

Probing black hole entropy via entanglement

Abstract

References in corpus (15)