Geometric entropy, area, and strong subadditivity
H. Casini
TL;DR
This paper shows that the geometric entropy of a vacuum state, defined by tracing over degrees of freedom in a spatial region, obeys an area law in relativistic quantum field theory, under general principles such as strong subadditivity, causality, and Poincaré symmetry. By analyzing Euclidean and Minkowski settings and introducing causally closed sets, the authors derive that the entropy for flat and polyhedral regions is governed by a boundary term proportional to area plus a possible constant; in higher dimensions the area term dominates, while the constant can be subtracted and does not affect the leading behavior. The results unify and generalize previous QFT computations, showing that the area-proportional growth is a universal feature of geometric entropy in the continuum limit, with potential implications for black hole entropy and covariant entropy bounds. The work delineates a rigorous, model-independent route to the area law via strong subadditivity and relativistic causality, clarifying the structure of divergences and offering a framework for broader region classes beyond spheres or half-spaces.
Abstract
The trace over the degrees of freedom located in a subset of the space transforms the vacuum state into a density matrix with non zero entropy. This geometric entropy is believed to be deeply related to the entropy of black holes. Indeed, previous calculations in the context of quantum field theory, where the result is actually ultraviolet divergent, have shown that the geometric entropy is proportional to the area for a very special type of subsets. In this work we show that the area law follows in general from simple considerations based on quantum mechanics and relativity. An essential ingredient of our approach is the strong subadditive property of the quantum mechanical entropy.
