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.