
TL;DR
This paper reviews the calculation of entanglement entropy in black holes, exploring mathematical tools, divergences, anomalies, and holographic perspectives, and discusses whether black hole entropy can be fully understood as entanglement entropy.
Contribution
It systematically analyzes the geometrical and quantum aspects of black hole entanglement entropy, highlighting the conical singularity method and its relation to other approaches.
Findings
Entanglement entropy is proportional to horizon area and depends on UV cutoff.
Logarithmic terms in entropy relate to conformal anomalies in 4 and 6 dimensions.
Holographic models illustrate the entanglement entropy of black hole horizons.
Abstract
The entanglement entropy is a fundamental quantity which characterizes the correlations between sub-systems in a larger quantum-mechanical system. For two sub-systems separated by a surface the entanglement entropy is proportional to the area of the surface and depends on the UV cutoff which regulates the short-distance correlations. The geometrical nature of the entanglement entropy calculation is particularly intriguing when applied to black holes when the entangling surface is the black hole horizon. I review a variety of aspects of this calculation: the useful mathematical tools such as the geometry of spaces with conical singularities and the heat kernel method, the UV divergences in the entropy and their renormalization, the logarithmic terms in the entanglement entropy in 4 and 6 dimensions and their relation to the conformal anomalies. The focus in the review is on the…
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