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Stability of Hybrid Higgs Inflation

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arxiv 2001.00154 v1 pith:V6Z3KIPB submitted 2020-01-01 gr-qc hep-th

Stability of Hybrid Higgs Inflation

classification gr-qc hep-th
keywords inflationhiggsmodelcouplinghybridcurvaturederivativeduring
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Hybrid Higgs inflation model is a hybrid type of the so-called Higgs inflation model with the conventional non-minimal $\xi$ coupling to a scalar curvature $R$ and new Higgs inflation model with the derivative coupling to the Einstein curvature tensor $G_{\mu\nu}$. This model can explain all possible value of the tensor-to-scalar ratio $r$ allowed by the present CMB constraints with an appropriate choice of coupling parameters. However the derivative coupling may causes a gradient instability during oscillation phase after inflation just as in new Higgs inflation model. Analyzing the behaviours of perturbations during oscillation phase in the hybrid Higgs inflation model, we show that the unstable scalar modes found in new Higgs inflation model are stabilized by the non-minimal $\xi$ coupling for some range of the coupling parameters.

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Cited by 2 Pith papers

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  1. Inflation with nondynamic distortion to leading order in slow roll

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    Nondynamic distortion integrated out of a 13-parameter metric-affine action sources the entire inflaton kinetic term; monomial models depend only on exponent ratio while α-attractors recover modified Starobinsky observables.

  2. Inflation with the Gauss-Bonnet term in the Palatini formulation

    astro-ph.CO 2026-03 accept novelty 5.0

    In Palatini gravity the inflaton–Gauss–Bonnet coupling yields a negative Chern–Simons-like kinetic correction and similar GW modifications, with metric-like behaviour unless the kinetic term nearly flips sign.