Finite Features of Quantum De Sitter Space
arXiv:2206.14146 · doi:10.1088/1361-6382/acaba5
Abstract
We consider degrees of freedom for a quantum de Sitter spacetime. The problem is studied from both a Lorentzian and a Euclidean perspective. From a Lorentzian perspective, we compute dynamical properties of the static patch de Sitter horizon. These are compared to dynamical features of black holes. We point out differences suggestive of non-standard thermal behaviour for the de Sitter horizon. We establish that geometries interpolating between an asymptotically AdS space and a dS interior are compatible with the null energy condition, albeit with a non-standard decreasing radial size of . The putative holographic dual of an asymptotic AdS spacetime is comprised of a finite number of degrees of freedom. From a Euclidean perspective we consider the gravitational path integral for fields over compact manifolds. In two-dimensions, we review Polchinski's BRST localisation of Liouville theory and propose a supersymmetric extension of timelike Liouville theory which exhibits supersymmetric localisation. We speculate that localisation of the Euclidean gravitational path integral is a reflection of a finite number of degrees of freedom in a quantum de Sitter universe.
20 pages plus appendices, published version including introduction + comment on fluid/gravity picture
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- The Cosmological Switchback Effect
- Complex geodesics in de Sitter space
- Keeping matter in the loop in dS quantum gravity
- A microscopic realization of dS
- Black hole to cosmic horizon microstates in string/M theory: timelike boundaries and internal averaging
- Late-Time Correlators and Complex Geodesics in de Sitter Space
- dS Supergravity
- Flat space gravity at finite cutoff
- Static sphere observers and geodesics in Schwarzschild-de Sitter spacetime
- The Cosmological Switchback Effect II
- Unconventional conformal invariance of maximal depth partially massless fields on and its relation to complex partially massless SUSY
- JT Gravity in de Sitter Space and Its Extensions