Jackiw-Teitelboim and Kantowski-Sachs quantum cosmology
arXiv:2112.00919 · doi:10.1088/1475-7516/2022/03/056
Abstract
We study quantum cosmology of the Jackiw-Teitelboim (JT) gravity with and calculate the Hartle-Hawking (HH) wave function for this model in the minisuperspace framework. Our approach is guided by the observation that the JT dynamics can be mapped exactly onto that of the Kantowski-Sachs (KS) model describing a homogeneous universe with spatial sections of topology. This allows us to establish a JT-KS correspondence between the wave functions of the models. We obtain the semiclassical Hartle-Hawking wave function by evaluating the path integral with appropriate boundary conditions and employing the methods of Picard-Lefschetz theory. The JT-KS connection formulas allow us to translate this result to JT gravity, define the HH wave function and obtain a probability distribution for the dilaton field.
arXiv comment43 pages, 6 figures
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- No smooth spacetime: Exploring primordial perturbations in Lorentzian quantum cosmology
- Aspects of Jackiw-Teitelboim Gravity in Anti-de Sitter and de Sitter spacetime
- JT Gravity in de Sitter Space and Its Extensions
- Functional Determinants for Constrained Path Integrals in Minisuperspace Jackiw-Teitelboim Gravity