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Quantum corrections to quartic inflation with a non-minimal coupling: metric vs. Palatini

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arxiv 1712.04874 v2 pith:JLW4HLD6 submitted 2017-12-13 gr-qc astro-ph.COhep-ph

classification gr-qcastro-ph.COhep-ph
keywords correctionseinsteinframequantumcurvedeffectivefieldgravity
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abstract

We study models of quartic inflation where the inflaton field $\phi$ is coupled non-minimally to gravity, $\xi \phi^2 R$, and perform a study of quantum corrections in curved space-time at one-loop level. We specifically focus on comparing results between the metric and Palatini theories of gravity. Transformation from the Jordan to the Einstein frame gives different results for the two formulations and by using an effective field theory expansion we derive the appropriate $\beta$-functions and the renormalisation group improved effective potentials in curved space for both cases in the Einstein frame. In particular, we show that in both formalisms the Einstein frame depends on the order of perturbation theory but that the flatness of the potential is unaltered by quantum corrections.

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Cited by 4 Pith papers

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  1. Infrared foundations for quantum geometry II: Catalogue of all torsion-like theories including new ghost-tachyon-free cases

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    A systematic catalogue of symmetric pair-antisymmetric rank-three field theories yields 22 ghost-tachyon-free models, all propagating vector torsion and none propagating scalar or pseudoscalar torsion.

  2. Parametric Resonance of Higgsed Vector Dark Matter: Inflationary Initial Conditions and Sourced Displacements

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    Stochastic inflationary fluctuations cannot supply the large dark-Higgs displacement required for broad parametric resonance production of vector dark matter, but a classically sourced Hubble-induced minimum can, with...

  3. Two-Measure Electroweak Standard Model. Some aspects of cosmological evolution and vacuum stability

    hep-th 2025-01 reject novelty 5.0 of 10

    The paper derives a two-measure version of the electroweak Standard Model in which couplings run classically with the cosmological background, giving small-xi Higgs inflation and a reparameterized fermion mass hierarchy.

  4. $\tilde\xi$-attractors in metric-affine gravity

    gr-qc 2024-11 conditional novelty 5.0 of 10

    A new class of metric-affine inflationary models, the ξ-tilde-attractors, reproduces Starobinsky inflation as a universal attractor in two strong-coupling limits.

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