How to count states in gravity
APA
(2026). How to count states in gravity. Perimeter Institute. https://pirsa.org/26040077
MLA
How to count states in gravity. Perimeter Institute, Apr. 02, 2026, https://pirsa.org/26040077
BibTex
@misc{ pirsa_PIRSA:26040077,
doi = {10.48660/26040077},
url = {https://pirsa.org/26040077},
author = {},
keywords = {Quantum Gravity},
language = {en},
title = {How to count states in gravity},
publisher = {Perimeter Institute},
year = {2026},
month = {apr},
note = {PIRSA:26040077 see, \url{https://pirsa.org}}
}
Abstract
Gibbons and Hawking proposed that the Euclidean gravity path integral with periodic boundary conditions in time computes the thermal partition sum of gravity. As a corollary, they argued that a derivative of the associated free energy with respect to the Euclidean time period computes gravitational entropy. Why is this interpretation correct? That is, why does this path integral compute a trace over the Hilbert space of quantum gravity? I will show that the quantity computed by the Gibbons-Hawking path integral is equal to an a priori different object -- an explicit thermal trace over the Hilbert space spanned by states produced by the Euclidean gravity path integral. I will explain that this follows if the Hilbert space with two boundaries factorizes into a product of two single boundary Hilbert spaces. To show the latter I will develop a basis for the nonperturbative Hilbert space of quantum gravity with one asymptotic boundary. I will use this basis to show that the Hilbert space for gravity with two disconnected boundaries factorizes into a product of two copies of the single boundary Hilbert space, from which our main result will follow.