The gravitational path integral from an observer's point of view

TL;DR

This paper develops a framework for describing the non-perturbative experience of a gravitating observer in quantum gravity, revealing a larger Hilbert space and resolving puzzles in black hole physics.

Contribution

It introduces a novel observer-centric approach to the gravitational path integral, expanding the Hilbert space and analyzing non-perturbative effects in black hole and cosmological spacetimes.

Findings

Hilbert space dimension scales exponentially with inverse Newton's constant.

Observer experiences non-trivial physics in closed universes.

Non-perturbative corrections in black holes are suppressed until exponential times in entropy.

Abstract

One of the fundamental problems in quantum gravity is to describe the experience of a gravitating observer in generic spacetimes. In this paper, we develop a framework for describing non-perturbative physics relative to an observer using the gravitational path integral. We apply our proposal to an observer that lives in a closed universe and one that falls behind a black hole horizon. We find that the Hilbert space that describes the experience of the observer is much larger than the Hilbert space in the absence of an observer. In the case of closed universes, the Hilbert space is not one-dimensional, as calculations in the absence of the observer suggest. Rather, its dimension scales exponentially with $G_N^{-1}$. Similarly, from an observer's perspective, the dimension of the Hilbert space in a two-sided black hole is increased. We compute various observables probing the experience of a gravitating observer in this Hilbert space. We find that an observer experiences non-trivial physics in the closed universe in contrast to what it would see in a one-dimensional Hilbert space. In the two-sided black hole setting, our proposal implies that non-perturbative corrections to effective field theory for an infalling observer are suppressed until times exponential in the black hole entropy, resolving a recently raised puzzle in black hole physics. While the framework that we develop is exemplified in the toy-model of JT gravity, most of our analysis can be extended to higher dimensions and, in particular, to generic spacetimes not admitting a conventional holographic description, such as cosmological universes or black hole interiors.