Emergence of Riemannian Quantum Geometry

TL;DR

This paper explores the emergence of quantum Riemannian geometry in loop quantum gravity, highlighting how space and spacetime are constructed from Planck-scale quantum grains through two complementary approaches.

Contribution

It presents a detailed comparison of continuum and discrete methods for deriving quantum geometry, clarifying their roles in loop quantum gravity.

Findings

Quantum geometry emerges from canonical quantization principles.

Discrete geometries encode finite degrees of freedom of gravity.

Both approaches complement each other in understanding quantum spacetime.

Abstract

In this chapter we take up the quantum Riemannian geometry of a spatial slice of spacetime. While researchers are still facing the challenge of observing quantum gravity, there is a geometrical core to loop quantum gravity that does much to define the approach. This core is the quantum character of its geometrical observables: space and spacetime are built up out of Planck-scale quantum grains. The interrelations between these grains are described by spin networks, graphs whose edges capture the bounding areas of the interconnected nodes, which encode the extent of each grain. We explain how quantum Riemannian geometry emerges from two different approaches: in the first half of the chapter we take the perspective of continuum geometry and explain how quantum geometry emerges from a few principles, such as the general rules of canonical quantization of field theories, a classical formulation of general relativity in which it appears embedded in the phase space of Yang-Mills theory, and general covariance. In the second half of the chapter we show that quantum geometry also emerges from the direct quantization of the finite number of degrees of freedom of the gravitational field encoded in discrete geometries. These two approaches are complimentary and are offered to assist readers with different backgrounds enter the compelling arena of quantum Riemannian geometry.