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Entanglement and local holography in quantum gravity

Published 4 Apr 2025 in hep-th, gr-qc, math-ph, math.MP, and quant-ph | (2504.03452v1)

Abstract: The It from Qubit paradigm proposes that gravitational spacetimes emerge from quantum entanglement. So far, the main evidence for this involves holographic dualities, where the entangled qubits live in a dual nongravitational theory. In this essay, we argue that string theory provides the mechanism to define these entangled qubits in the bulk gravitating theory. This involves a local form of geometric transition, which is the stringy mechanism that underlies \emph{local} holography. We illustrate how this works in the A model topological string,

Summary

Entanglement and Local Holography in Quantum Gravity

The paper "Entanglement and Local Holography in Quantum Gravity" by Gabriel Wong argues for a novel understanding of how gravitational spacetimes can emerge from quantum entanglement—specifically within the framework of string theory. The central thesis is that closed strings in gravitational backgrounds can be conceptualized as entangled pairs of open strings within a background of branes and antibranes, which embodies a local realization of the holographic principle.

Key Concepts

The discussion begins by elaborating on the "It from Qubit" paradigm, which posits that spacetime geometry emerges from quantum entanglement. This has been most prominently explored in the context of AdS/CFT duality. However, the paper seeks to extend beyond these established dualities by focusing on the string theory mechanisms that enable such an emergence directly in the bulk gravitational theory.

Factorization Challenge in Quantum Gravity:

In quantum field theory (QFT), entanglement entropy can be defined via a factorization of the Hilbert space into subregions, formalized by a factorization map. However, gravitational systems pose additional challenges due to their diffeomorphism-invariant nature, raising the question of how to define this factorization in the context of fluctuating spacetimes.

The paper proposes that string theory offers a solution through geometric transitions, which effectively factorize the bulk closed-string Hilbert space. String theory edge modes play a pivotal role analogous to how edge modes resolve ambiguities in gauge theories.

Local Holography and Shrinkable Boundaries

The paper emphasizes local holography—a string-theory-driven reduction of space into holographic information encoded on a lower-dimensional structure. A focus is given to the quantum field theoretic treatment of Euclidean path integrals and the introduction of a "shrinkable" boundary condition, which preserves the entanglement entropy while ensuring that quantum gravity constraints are met.

Application in Topological String Theory

The paper illustrates these concepts using the A-model of topological string theory, where entanglement branes provide a mechanism for factorization. These branes serve as discrete, quantum-deformed boundaries that allow for the factorization of the closed string amplitudes into open string sectors. The critical mathematical tool here is the "quantum trace," which handles the non-commuting properties inherent in quantum groups.

In particular, the quantum trace captures the entanglement inherent in the Chan-Paton factors of D-branes, offering a microscopic handle on how gravitational entropy can emerge at large N limits.

Implications and Speculative Outlook

This string-theoretic approach suggests a deep connection between geometric transitions and entanglement entropy in quantum gravity, potentially providing insights into the interpretation of gravitational entropy as entropic quantities emergent from bulk quantities. This line of reasoning opens avenues for exploring the nature of quantum gravitational degrees of freedom, particularly in cosmological scenarios such as de Sitter spacetime, where traditional boundary methods are inapplicable.

Moreover, the paper eludes to the connection between the shrinkability condition and the cobordism conjecture, conjecturing that the existence of certain gravitational cobordism objects are crucial for capturing the full spectrum of entangled states and thereby the true entropy of quantum gravitational systems.

In conclusion, this work enriches the dialogue between quantum field theory, general relativity, and string theory, providing a fresh lens on how entanglement might bridge these domains to a more unified understanding of quantum gravity. Future research could refine these theoretical frameworks, potentially leading to new paradigms for understanding space-time, entanglement, and, most fundamentally, the universe's quantum mechanical underpinnings.

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