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The Higgs field as an inflaton

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arxiv 1307.0708 v2 pith:CRIF4J5A submitted 2013-07-02 hep-ph gr-qchep-th

Fedor Bezrukov This is my paper · ORCID
classification hep-phgr-qchep-th
keywords higgsmodelfieldagreementarisingbackgroundbosonclosely
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The Higgs field of the pure Standard Model can lead to the inflationary expansion of the early Universe if it is non-minimally coupled to gravity. The model predicts Cosmic Microwave Background (CMB) parameters in perfect agreement with the current observations and has implications for the Higgs boson mass. We review the model, its predictions, problems arising with its quantization and some closely related models.

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Cited by 4 Pith papers

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

  1. Precision Unitarity Calculations in Inflationary Models

    hep-ph 2025-05 conditional novelty 7.0 of 10

    Full S-matrix unitarity calculations show the cut-off in single-field nonminimal inflation rises to about 20 M_Pl/ξ for small couplings, while multifield kinetic interactions keep the cut-off near M_Pl/ξ.

  2. Implication of preheating on gravity assisted baryogenesis in $R^2$-Higgs inflation

    hep-ph 2024-11 conditional novelty 6.0 of 10

    Preheating in R2-Higgs inflation sets the reheating temperature, and matching the observed baryon asymmetry fixes the baryogenesis scale to about 2.1 to 2.8 x 10^-5 M_Planck for xi_H between 1 and 10.

  3. Non-Standard Thermal History and Formation of Primordial Black Holes in Einstein-Gauss-Bonnet Gravity

    gr-qc 2025-01 conditional novelty 5.0 of 10

    A tuned Einstein-Gauss-Bonnet inflation model can create primordial black holes from asteroid-sized to tens of solar masses and secondary gravitational waves, with abundances that change dramatically in a stiff post-i...

  4. Gravitational waves from a first-order phase transition of the inflaton

    hep-ph 2024-12 conditional novelty 5.0 of 10

    A single non-minimally coupled dark Higgs can drive both inflation and a first-order phase transition whose gravitational waves fall within the reach of planned experiments.

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