Higgs Chaotic Inflation in Standard Model and NMSSM
  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. For instance, the inflaton potential is
proportional to phi^2 and phi^{2/3} in the standard model and NMSSM,
respectively. It is also possible to have a flatter inflaton potential.
