Formulation and Proof of the Gravitational Entropy Bound

TL;DR

This paper formulates and proves a gravitational entropy bound within a quantum phase space framework, linking the bound to the area of a surface and demonstrating its validity for Einstein-Hilbert gravity with matter.

Contribution

It introduces a novel formulation and proof of the gravitational entropy bound using a phase space approach and diffeomorphism invariance, explicitly relating the bound to surface area.

Findings

The entropy bound is expressed as (V) ^{rac{}{\u03b5}} ",

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Abstract

We provide a formulation and proof of the gravitational entropy bound. We use a recently given framework which expresses the measurable quantities of a quantum theory as a weighted sum over paths in the theory's phase space. If this framework is applied to a field theory on a spacetime foliated by a hypersurface $\Sigma,$ the choice of a codimension-2 surface $B$ without boundary contained in $\Sigma$ specifies a submanifold in the phase space. We show here that this submanifold is naturally restricted to obey an entropy bound if the field theory is diffeomorphism-invariant. We prove this restriction to arise by considering the quantum-mechanical sum of paths in phase space and exploiting the interplay of the commutativity of the sum with diffeomorphism-invariance. The formulation of the entropy bound, which we state and derive in detail, involves a functional $K$ on the submanifold associated to $B.$ We give an explicit construction of $K$ in terms of the Lagrangian. The gravitational entropy bound then states: For any real $\frac{\lambda}{\hbar},$ consider the set of states where $K$ takes a value not bigger than $\lambda$ and let $V$ denote the phase space volume of this set. One has then $\ln (V) \le \frac{\lambda}{\hbar}.$ Especially, we show for the Einstein-Hilbert Lagrangian in any dimension with cosmological constant and arbitrary minimally coupled matter, one has $K = \frac{A}{4G}.$ Hereby, $A$ denotes the area of $B$ in a particular state.