Low-curvature quantum corrections from unitary evolution of de Sitter space

Abstract We study the quantum dynamics of de Sitter space formulated as a minisuperspace model with flat spatial hypersurfaces in unimodular gravity, both in the Wheeler–DeWitt approach and in loop quantum cosmology. Time evolution is defined naturally in unimodular time, which appears as conjugate to the cosmological (integration) constant. We show that requiring unitary time evolution ‘resolves’ the de Sitter horizon where the flat slicing breaks down and leads to strong quantum effects there, even though locally nothing special happens at this surface. For a cosmological constant that is far below the Planck scale, loop quantum gravity corrections do not alter the main results in any substantial way. This model illustrates the fundamental clash between general covariance and unitarity in quantum gravity.

Authors

Publication Details

Journal
Classical and Quantum Gravity
Published
2025-04-03
DOI
https://doi.org/10.1088/1361-6382/adc8f3
Citations
2
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
3.74

Funders

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article

Low-curvature quantum corrections from unitary evolution of de Sitter space

Steffen Gielen, Rita B. Neves
2 citations
Classical and Quantum Gravity
Black Holes and Theoretical Physics
3.74
article

Low-curvature quantum corrections from unitary evolution of de Sitter space

Steffen Gielen, Rita B. Neves
article en
2 citations

Abstract

Abstract We study the quantum dynamics of de Sitter space formulated as a minisuperspace model with flat spatial hypersurfaces in unimodular gravity, both in the Wheeler–DeWitt approach and in loop quantum cosmology. Time evolution is defined naturally in unimodular time, which appears as conjugate to the cosmological (integration) constant. We show that requiring unitary time evolution ‘resolves’ the de Sitter horizon where the flat slicing breaks down and leads to strong quantum effects there, even though locally nothing special happens at this surface. For a cosmological constant that is far below the Planck scale, loop quantum gravity corrections do not alter the main results in any substantial way. This model illustrates the fundamental clash between general covariance and unitarity in quantum gravity.

Classical and Quantum GravityVol. 42(14)
Royal Society
Openalex Percentile: Top 9%
Black Holes and Theoretical Physics
3.74
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