Higgs chaotic inflation in standard model and NMSSM

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43 Citations (Scopus)


We construct a chaotic inflation model in which the Higgs fields play the role of the inflaton in the standard model as well as in the singlet extension of the supersymmetric standard model. The key idea is to allow a non-canonical kinetic term for the Higgs field. The model is a realization of the recently proposed running kinetic inflation, in which the coefficient of the kinetic term grows as the inflaton field. The inflaton potential depends on the structure of the Higgs kinetic term. In the simplest cases, the inflaton potential is proportional to φ2 and φ2/3 in the standard model and NMSSM, respectively.

Original languageEnglish
Article number010
JournalJournal of Cosmology and Astroparticle Physics
Issue number2
Publication statusPublished - 2011 Feb
Externally publishedYes


  • inflation
  • supersymmetry and cosmology

ASJC Scopus subject areas

  • Astronomy and Astrophysics


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