On the Euclidean action of de Sitter black holes and constrained instantons
Edward K. Morvan, Jan Pieter van der Schaar, Manus R. Visser
SciPost Phys. 14, 022 (2023) · published 23 February 2023
- doi: 10.21468/SciPostPhys.14.2.022
We compute the on-shell Euclidean action of Schwarzschild-de Sitter black holes, and take their contributions in the gravitational path integral into account using the formalism of constrained instantons. Although Euclidean de Sitter black hole geometries have conical singularities for generic masses, their on-shell action is finite and is shown to be independent of the Euclidean time periodicity and equal to minus the sum of the black hole and cosmological horizon entropy. We apply this result to compute the probability for a nonrotating, neutral arbitrary mass black hole to nucleate spontaneously in empty de Sitter space, which separates into a constant and a "non-perturbative" contribution, the latter corresponding to the proper saddle-point instanton in the Nariai limit. We also speculate on some further applications of our results, most notably as potential non-perturbative corrections to correlators in the de Sitter vacuum.
Cited by 1
Pasquarella et al., Vacuum transitions in two-dimensions and their holographic interpretation
J. High Energ. Phys. 2023, 192 (2023) [Crossref]
Authors / Affiliations: mappings to Contributors and OrganizationsSee all Organizations.
- 1 2 Edward K. Morvan,
- 1 2 Jan Pieter van der Schaar,
- 3 Manus R. Visser
- 1 Institute of Physics, University of Amsterdam [IoP, UvA]
- 2 Delta Institute for Theoretical Physics [Delta ITP]
- 3 Université de Genève / University of Geneva [UNIGE]