Cosmological Perturbations in the New Higgs Inflation
  We study the cosmological perturbations created during the New Higgs
inflationary phase. In the New Higgs Inflation, the Higgs boson is kinetically
coupled to the Einstein tensor and only three perturbative degrees of freedom,
a scalar and two tensorial (gravitational waves), propagate during Inflation.
Scalar perturbations are found to match the latest WMAP-7yrs data within
Standard Model Higgs parameters. Primordial gravitational waves also, although
propagating with superluminal speed, are consistent with present data. Finally,
we estimate the values of the parameter of the New Higgs Inflation in relation
to the Higgs mass, the spectral index and amplitude of the primordial scalar
perturbations showing that the unitarity bound of the theory is not violated.
