Global quenches and correlator dynamics in de Sitter space

We study nonequilibrium initial states of quantum fields in curved spacetime and develop a framework for describing global quenches as unitary perturbations of the initial density matrix. Using the Keldysh-Schwinger functional integral, we derive expressions for postquench correlators in arbitrary geometries and apply the method to both Minkowski and de Sitter backgrounds. In flat space, the approach reproduces the known relaxation behavior for massive fields and reveals qualitatively distinct dynamics in the massless case. In de Sitter space, we find that the late-time decay of quench-induced corrections depends sensitively on the mass and may influence the behavior of cosmological observables such as the power spectrum. The framework also extends straightforwardly to non-Gaussian initial states, providing a basis for future studies of loop effects and primordial non-Gaussianities.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2026-03-09
DOI
https://doi.org/10.1103/7tq5-bkn3
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
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article

Global quenches and correlator dynamics in de Sitter space

Anonymous
Physical review. D/Physical review. D.
Black Holes and Theoretical Physics
article

Global quenches and correlator dynamics in de Sitter space

Anonymous
article en

Abstract

We study nonequilibrium initial states of quantum fields in curved spacetime and develop a framework for describing global quenches as unitary perturbations of the initial density matrix. Using the Keldysh-Schwinger functional integral, we derive expressions for postquench correlators in arbitrary geometries and apply the method to both Minkowski and de Sitter backgrounds. In flat space, the approach reproduces the known relaxation behavior for massive fields and reveals qualitatively distinct dynamics in the massless case. In de Sitter space, we find that the late-time decay of quench-induced corrections depends sensitively on the mass and may influence the behavior of cosmological observables such as the power spectrum. The framework also extends straightforwardly to non-Gaussian initial states, providing a basis for future studies of loop effects and primordial non-Gaussianities.

Physical review. D/Physical review. D.Vol. 113(6)
P.N. Lebedev Physical Institute of the Russian Academy of Sciences (RU), Moscow Institute of Physics and Technology (RU)
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Black Holes and Theoretical Physics
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Global quenches and correlator dynamics in de Sitter space — Anonymous · Physical review. D/Physical review. D. (2026) | TGRS Research Map | TGRS