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Scalar field correlator in de Sitter space at next-to-leading order in a 1/N expansion

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arxiv 1509.05546 v2 pith:WJAVHTHX submitted 2015-09-18 hep-th gr-qchep-phnucl-th

classification hep-thgr-qchep-phnucl-th
keywords expansionsittercorrelatorfieldinfraredmassnext-to-leadingorder
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We study the dynamics of light quantum scalar fields in de Sitter space on superhorizon scales. We compute the self-energy of an O(N) symmetric theory at next-to-leading order in a 1/N expansion in the regime of superhorizon momenta, and we obtain an exact analytical solution of the corresponding Dyson-Schwinger equations for the two-point correlator. This amounts to resumming the infinite series of nonlocal self-energy insertions, which typically generate spurious infrared and/or secular divergences. The potentially large de Sitter logarithms resum into well-behaved power laws from which we extract the field strength and mass renormalization. The nonperturbative 1/N expansion allows us to discuss the case of vanishing and negative tree-level square mass, which both correspond to strongly coupled effective theories in the infrared.

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  1. Spontaneous symmetry breaking induced by curvature : Analysis via non-perturbative 2PI Hartree approximation

    gr-qc 2025-04 conditional novelty 6.0 of 10

    Curvature, via resummed 2PI Hartree self-energy, can induce spontaneous symmetry breaking for a minimally coupled scalar with positive mass squared in de Sitter spacetime.

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