Remarks on 2D quantum cosmology

Abstract We consider two-dimensional quantum gravity endowed with a positive cosmological constant and coupled to a conformal field theory of large and positive central charge. We study cosmological properties at the classical and quantum level. We provide a complete ADM analysis of the classical phase space, revealing a family of either bouncing or big bang/crunch type cosmologies. At the quantum level, we solve the Wheeler-DeWitt equation exactly. In the semiclassical limit, we link the Wheeler-DeWitt state space to the classical phase space. Wavefunctionals of the Hartle-Hawking and Vilenkin type are identified, and we uncover a quantum version of the bouncing spacetime. We retrieve the Hartle-Hawking wavefunction from the disk path integral of timelike Liouville theory. To do so, we must select a particular contour in the space of complexified fields. The quantum information content of the big bang cosmology is discussed, and contrasted with the de Sitter horizon entropy as computed by a gravitational path integral over the two-sphere.

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Publication Details

Journal
Journal of Cosmology and Astroparticle Physics
Published
2024-10-01
DOI
https://doi.org/10.1088/1475-7516/2024/10/031
Citations
16
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
10.55

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article

Remarks on 2D quantum cosmology

Beatrix Mühlmann, Dionysios Anninos, Chiara Baracco
16 citations
Journal of Cosmology and Astroparticle Physics
Black Holes and Theoretical Physics
10.55
article

Remarks on 2D quantum cosmology

Beatrix Mühlmann, Dionysios Anninos, Chiara Baracco
article en
16 citations

Abstract

Abstract We consider two-dimensional quantum gravity endowed with a positive cosmological constant and coupled to a conformal field theory of large and positive central charge. We study cosmological properties at the classical and quantum level. We provide a complete ADM analysis of the classical phase space, revealing a family of either bouncing or big bang/crunch type cosmologies. At the quantum level, we solve the Wheeler-DeWitt equation exactly. In the semiclassical limit, we link the Wheeler-DeWitt state space to the classical phase space. Wavefunctionals of the Hartle-Hawking and Vilenkin type are identified, and we uncover a quantum version of the bouncing spacetime. We retrieve the Hartle-Hawking wavefunction from the disk path integral of timelike Liouville theory. To do so, we must select a particular contour in the space of complexified fields. The quantum information content of the big bang cosmology is discussed, and contrasted with the de Sitter horizon entropy as computed by a gravitational path integral over the two-sphere.

Journal of Cosmology and Astroparticle PhysicsVol. 2024(10)
King's College London (GB), King's College School (GB), McGill University (CA), KU Leuven (BE)
Science and Technology Facilities Council
Sustainable cities and communities
Openalex Percentile: Top 1%
Black Holes and Theoretical Physics
10.55
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