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Infrared dynamics in de Sitter space from Schwinger-Dyson equations

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arxiv 1305.5705 v2 pith:VVN5ZHFN submitted 2013-05-24 hep-th gr-qchep-phnucl-th

classification hep-thgr-qchep-phnucl-th
keywords infraredequationsschwinger-dysoncorrelatorlawsmassmomentapower
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We study the two-point correlator of an O(N) scalar field with quartic self-coupling in de Sitter space. For light fields in units of the expansion rate, perturbation theory is plagued by large logarithmic terms for superhorizon momenta. We show that a proper treatment of the infinite series of self-energy insertions through the Schwinger-Dyson equations resums these infrared logarithms into well defined power laws. We provide an exact analytical solution of the Schwinger-Dyson equations for infrared momenta when the self-energy is computed at two-loop order. The obtained correlator exhibits a rich structure with a superposition of free-field-like power laws. We extract mass and field-strength renormalization factors from the asymptotic infrared behavior. The latter are nonperturbative in the coupling in the case of a vanishing tree-level mass.

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  1. From the Fokker-Planck equation to perturbative QFT's results in de Sitter space

    hep-th 2025-04 accept novelty 6.0 of 10

    An iterative Fokker-Planck scheme reproduces the known perturbative two- and four-point correlation functions of a self-interacting spectator scalar field in de Sitter space.

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