# Quantum gravity in timeless configuration space

## TL;DR

This paper proposes a novel approach to quantum gravity by encoding it in a timeless configuration space, leading to emergent time and a Schrödinger-like evolution that avoids common issues in traditional quantum gravity formalisms.

## Contribution

It introduces a framework where boundary conditions are derived from fundamental principles, resulting in a unique reduced configuration space and emergent time, applicable to theories like shape dynamics.

## Key findings

- Derives a Schrödinger equation in the classical limit for weakly coupled fields.
- Provides a method to calculate gravitational semi-classical probabilities.
- Avoids the multiple solution problem of standard WKB in quantum gravity.

## Abstract

On the path towards quantum gravity, we find friction between temporal relations in quantum mechanics (QM) (where they are fixed and field-independent), and in general relativity (where they are field-dependent and dynamic). This paper aims to attenuate that friction, by encoding gravity in the timeless configuration space of spatial fields with dynamics given by a path integral. The framework demands that boundary conditions for this path integral be uniquely given, but unlike other approaches where they are prescribed --- such as the no-boundary and the tunneling proposals --- here I postulate basic principles to identify boundary conditions in a large class of theories. Uniqueness arises only if a reduced configuration space can be defined and if it has a profoundly asymmetric fundamental structure. These requirements place strong restrictions on the field and symmetry content of theories encompassed here; shape dynamics is one such theory. Also as in other boundary proposals, Time, including space-time, emerges as an effective concept; valid for certain curves in configuration space but not assumed from the start. When some such notion of time becomes available, conservation of (positive) probability currents ensues. I show that, in the appropriate limits, a Schroedinger equation dictates the evolution of weakly coupled source fields on a classical gravitational background. Due to the asymmetry of reduced configuration space, these probabilities and currents avoid a known difficulty of standard WKB approximations for Wheeler DeWitt in minisuperspace: the selection of a unique Hamilton-Jacobi solution to serve as background. I illustrate these constructions with a simple example of a full quantum gravitational theory (i.e. not in minisuperspace) for which the formalism is applicable, and give a formula for calculating gravitational semi-classical relative probabilities in it.