Algebras and Hilbert spaces from gravitational path integrals: Understanding Ryu-Takayanagi/HRT as entropy without AdS/CFT
Eugenia Colafranceschi, Xi Dong, Donald Marolf, Zhencheng Wang
TL;DR
The paper shows that in any UV-complete bulk gravity with a Euclidean path integral satisfying simple axioms, boundary observables organize into type I von Neumann algebras that are mutual commutants, yielding a Hilbert-space interpretation of the Ryu-Takayanagi entropy. By constructing left/right surface algebras and their representations on a diagonal boundary Hilbert space, the authors derive a discrete sector decomposition indexed by μ and demonstrate a tensor product factorization of the corresponding Hilbert spaces, enabling RT/HRT to be computed as standard traces with quantum corrections in semiclassical limits. A key innovation is the introduction of hidden sectors, quantization of projection traces, and a gravitational replica trick that recovers RT entropy while remaining fully within a bulk, holography-free framework. The framework is illustrated with explicit 2d models (topological gravity and JT gravity, with and without matter) and clarifies how islands and entropy mixing arise from algebraic structures, while also showing how semiclassical limits can violate assumptions if the axioms are not maintained. Overall, this approach provides a robust, UV-complete, bulk-based interpretation of gravitational entropy and suggests broad applicability to various UV completions of quantum gravity beyond AdS/CFT.
Abstract
Recent works by Chandrasekaran, Penington, and Witten have shown in various special contexts that the quantum-corrected Ryu-Takayanagi (RT) entropy (or its covariant Hubeny-Rangamani-Takayanagi (HRT) generalization) can be understood as computing an entropy on an algebra of bulk observables. These arguments do not rely on the existence of a local holographic dual field theory. We show that analogous-but-stronger results hold in any UV-completion of asymptotically AdS quantum gravity with a Euclidean path integral satisfying a simple and (largely) familiar set of axioms. We consider a quantum context in which a standard Lorentz-signature classical bulk limit would have Cauchy slices with asymptotic boundaries $B_L \sqcup B_R$ where both $B_L$ and $B_R$ are compact manifolds without boundary. Our main result is that (the UV-completion of) the quantum gravity path integral defines type I von Neumann algebras ${\cal A}^{B_L}_L$, ${\cal A}^{B_R}_{R}$ of observables acting respectively at $B_L$, $B_R$ such that ${\cal A}^{B_L}_L$, ${\cal A}^{B_R}_{R}$ are commutants. The path integral also defines entropies on ${\cal A}^{B_L}_L, {\cal A}^{B_R}_R$. Positivity of the Hilbert space inner product then turns out to require the entropy of any projection operator to be quantized in the form $\ln N$ for some $N \in {\mathbb Z}^+$ (unless it is infinite). As a result, our entropies can be written in terms of standard density matrices and standard Hilbert space traces. Furthermore, in appropriate semiclassical limits our entropies are computed by the RT-formula with quantum corrections. Our work thus provides a Hilbert space interpretation of the RT entropy. Since our axioms do not severely constrain UV bulk structures, it is plausible that they hold equally well for successful formulations of string field theory, spin-foam models, or any other approach to constructing a UV-complete theory of gravity.
