Schwarzschild Black Holes and Asymptotic
arXiv:1805.06079
Abstract
We show that the entropy of D--dimensional Schwarzschild black holes are given by the entanglement entropy of a boundary of global space that lives at asymptotic infinity. We dimensionally reduce General Relativity to two dimensions which leads to 2D dilatonic gravity which has black hole solutions with the same thermodynamics as D--dimensional Schwarzschild black holes. These dilatonic black holes can be transformed into certain black holes by Weyl transformations which are symmetries of the theory that preserve the thermodynamics. In the asymptotic limit, the black holes become global which can be described by two entangled Rindler spaces. The entanglement entropy of a single Rindler space reproduces the Schwarzschild black hole entropy.
20 pages
References in corpus (15)
- Comments on the Sachdev-Ye-Kitaev model
- Near-horizon symmetries of extremal black holes
- Holographic Entanglement Entropy
- Near Extremal Black Hole Entropy as Entanglement Entropy via AdS2/CFT1
- Extremal vacuum black holes in higher dimensions
- Ads(3)/CFT(2) to Ads(2)/CFT(1)
- Conformal symmetry and its breaking in two dimensional Nearly Anti-de-Sitter space
- Black Holes as Conformal Field Theories on Horizons
- Horizon Conformal Field Theories from Black Holes
- Rindler Energy is Wald Entropy
- Gravitational Entropy and String Bits on the Stretched Horizon
- Liouville Theory on Horizons: Towards a Quantum Theory of Black Holes
- On the Holographic Nature Of Rindler Energy
- Extremal Black Hole Entropy from Horizon Conformal Field Theories
- The Holographic Entanglement Entropy of Schwarzschild Black Holes