Closed universes in two dimensional gravity
arXiv:2402.00098 · doi:10.21468/SciPostPhys.17.2.051
Abstract
We study closed universes in simple models of two dimensional gravity, such as Jackiw-Teiteilboim (JT) gravity coupled to matter, and a toy topological model that captures the key features of the former. We find there is a stark contrast, as well as some connections, between the perturbative and non-perturbative aspects of the theory. We find rich semi-classical physics. However, when non-perturbative effects are included there is a unique closed universe state in each theory. We discuss possible meanings and interpretations of this observation.
v1: 25+16 pages, 13 figures; v2: references added; v3: published version
References in corpus (15)
- An Algebra of Observables for de Sitter Space
- Solvable Models of Quantum Black Holes: A Review on Jackiw-Teitelboim Gravity
- More quantum noise from wormholes
- Gravity factorized
- Wormholes without averaging
- Accelerating cosmology from a holographic wormhole
- Double-scaled SYK and de Sitter Holography
- De Sitter Space, Double-Scaled SYK, and the Separation of Scales in the Semiclassical Limit
- A Paradox and its Resolution Illustrate Principles of de Sitter Holography
- Infinite Temperature's Not So Hot
- Gauging spacetime inversions in quantum gravity
- Non-perturbative de Sitter Jackiw-Teitelboim gravity
- Constructing all BPS black hole microstates from the gravitational path integral
- Bit models of replica wormholes
- A note on background independence in string theory