Microscopic count of de Sitter horizon entropy · revision history
Revision 1
Accepted · first revision · record
- Title
- Microscopic count of de Sitter horizon entropy
- Plain
- The horizon of an expanding universe has an entropy proportional to its area, just like a black hole. Which quantum states it counts is unknown.
- Precise
- The Gibbons-Hawking entropy of a d-dimensional de Sitter horizon is $S = A c^3/(4 G \hbar)$ with $k_B = 1$. Find a statistical system whose state count reproduces S including the one-loop logarithmic correction computed by Anninos, Denef, Law and Sun (2020).
- Settled by
- A microscopic system with a derived match of the leading area term and the logarithmic correction.
- Kind
- well-posed
- Answer type
- identification
- References
- (empty)
- Literature status
- open
- Status note
- The static-patch algebra of observables was shown to be of von Neumann type $\mathrm{II}_{1}$ with a maximum-entropy state (Chandrasekaran, Longo, Penington, Witten 2022), without a microscopic count.
- Posed since
- 1977