Abstract

We construct a model of quantum gravity in which dimension, topology and geometry of spacetime are dynamical. The microscopic degree of freedom is a real rectangular matrix whose rows label internal flavours, and columns label spatial sites. In the limit that the size of the matrix is large, the sites can collectively form a spatial manifold. The manifold is determined from the pattern of entanglement present across local Hilbert spaces associated with column vectors of the matrix. With no structure of manifold fixed in the background, the spacetime gauge symmetry is generalized to a group that includes diffeomorphism in arbitrary dimensions. The momentum and Hamiltonian that generate the generalized diffeomorphism obey a first-class constraint algebra at the quantum level. In the classical limit, the constraint algebra of the general relativity is reproduced as a special case. The first-class nature of the algebra allows one to express the projection of a quantum state of the matrix to a gauge invariant state as a path integration of dynamical variables that describe collective fluctuations of the matrix. The collective variables describe dynamics of emergent spacetime, where multi-fingered times arise as Lagrangian multipliers that enforce the gauge constraints. If the quantum state has a local structure of entanglement, a smooth spacetime with well-defined dimension, topology, signature and geometry emerges at the saddle-point, and the spin two mode that determines the geometry can be identified. We find a saddle-point solution that describes a series of (3 + 1)-dimensional de Sitter-like spacetimes with the Lorentzian signature bridged by Euclidean spaces in between. The phase transitions between spacetimes with different signatures are caused by Lifshitz transitions in which the pattern of entanglement is rearranged across the system. Fluctuations of the collective variables are described by bi-local fields that propagate in the spacetime set up by the saddle-point solution.

Highlights

  • According to Einstein’s theory of general relativity, gravity originates from dynamical geometry [1]

  • In the background independent model, the collective variables that describe dynamics of dimension, topology and geometry are classical in the large N limit, where N is the number of flavours of underlying quantum matter [34]

  • We present a model for a background independent quantum gravity in which dimension, topology and geometry are all dynamical

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Summary

Introduction

According to Einstein’s theory of general relativity, gravity originates from dynamical geometry [1]. A background independent non-perturbative formulation of the string theory is not known yet, the AdS/CFT correspondence already provides an important clue on the microscopic origin of gravity : geometry is nothing but a coarse-grained variable that controls entanglement (among other things) of ordinary quantum matter [26,27,28,29,30,31,32]. The connectivity, in turn, determines a manifold, if its pattern exhibits a local structure Within this framework, a Hamiltonian that governs the dynamics of the underlying quantum matter naturally induces dynamics of collective variables that describe dimension, topology and geometry of the manifold. In the background independent model, the collective variables that describe dynamics of dimension, topology and geometry are classical in the large N limit, where N is the number of flavours of underlying quantum matter [34]. For other related approaches to quantum gravity, see refs. [33, 35,36,37,38]

Conceptual overview
Outline
Hilbert space
Local structure
Gauge symmetry
Momentum constraint
Hamiltonian constraint
First-class constraint algebra
Projection
Gauge invariant local structure
Path integration of collective variables
Gauge invariance of the action
Spacetime diffeomorphism and emergent geometry
Momentum density
Hamiltonian density
Emergent metric
Symmetry of semi-classical states
Saddle-point equation of motion
Gauge fixing
Translationally invariant solution
Numerical solution
Analytic solution
Emergent Lorentz symmetry
Effective theory
Summary and discussion
Open questions
Full Text
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