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Higgs-portal assisted Higgs inflation with a sizeable tensor-to-scalar ratio

  • Jinsu Kim*
  • , Pyungwon Ko
  • , Wan Il Park
  • *Corresponding author for this work
  • Korea Institute for Advanced Study
  • University of Valencia

Research output: Contribution to journalJournal articlepeer-review

Abstract

We show that the Higgs portal interactions involving extra dark Higgs field can save generically the original Higgs inflation of the standard model (SM) from the problem of a deep non-SM vacuum in the SM Higgs potential. Specifically, we show that such interactions disconnect the top quark pole mass from inflationary observables and allow multi-dimensional parameter space to save the Higgs inflation, thanks to the additional parameters (the dark Higgs boson mass mφ, the mixing angle α between the SM Higgs H and dark Higgs Φ, and the mixed quartic coupling) affecting RG-running of the Higgs quartic coupling. The effect of Higgs portal interactions may lead to a larger tensor-to-scalar ratio, 0.08 ≲ r ≲ 0.1, by adjusting relevant parameters in wide ranges of α and mφ, some region of which can be probed at future colliders. Performing a numerical analysis we find an allowed region of parameters, matching the latest Planck data.

Original languageEnglish
Article number003
JournalJournal of Cosmology and Astroparticle Physics
Volume2017
Issue number2
DOIs
StatePublished - 2017.02.1

Keywords

  • ination
  • particle physics-cosmology connection
  • physics of the early universe

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