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Hybrid Higgs Inflation: The Use of Disformal Transformation

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arxiv 1712.04237 v2 pith:MSO6MG26 submitted 2017-12-12 gr-qc astro-ph.COhep-phhep-th

Hybrid Higgs Inflation: The Use of Disformal Transformation

classification gr-qc astro-ph.COhep-phhep-th
keywords higgsmodelhybridinflationconventionalcouplingdisformalframe
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We propose a hybrid type of the conventional Higgs inflation and new Higgs inflation models. We perform a disformal transformation into the Einstein frame and analyze the background dynamics and the cosmological perturbations in the truncated model, in which we ignore the higher-derivative terms of the Higgs field. From the observed power spectrum of the density perturbations, we obtain the constraint on the non-minimal coupling constant $\xi$ and the mass parameter $M$ in the derivative coupling. Although the primordial tilt $n_s$ in the hybrid model barely changes, the tensor-to-scalar ratio $r$ moves from the value in new Higgs inflationary model to that in the conventional Higgs inflationary model as $|\xi|$ increases. We confirm our results by numerical analysis by ADM formalism of the full theory in the Jordan frame.

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Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

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  2. Robustness of Starobinsky inflation in a minimal two-field scalar-tensor completion

    gr-qc 2026-04 conditional novelty 6.0

    A minimal two-field radiative completion of Starobinsky inflation remains observably indistinguishable from the original model on the studied attractor-connected slow-roll branch.

  3. 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.

  4. Robustness of Starobinsky inflation in a minimal two-field scalar-tensor completion

    gr-qc 2026-04 unverdicted novelty 4.0

    In this two-field completion, trajectories connected to the Starobinsky solution keep entropy modes suppressed so that curvature and tensor perturbations remain effectively single-field Starobinsky-like.

  5. Robustness of Starobinsky inflation in a minimal two-field scalar-tensor completion

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    Nearby trajectories in a minimal two-field scalar-tensor completion of Starobinsky inflation relax to an attractor where entropy sourcing is negligible, so observables remain effectively Starobinsky-like.