Bounce Inflation Cosmology with Standard Model Higgs Boson
  It is of great interest to connect cosmology in the early universe to the
Standard Model of particle physics. In this paper, we try to construct a bounce
inflation model with the standard model Higgs boson, where the one loop
correction is taken into account in the effective potential of Higgs field. In
this model, a Galileon term has been introduced to eliminate the ghost mode
when bounce happens. Moreover, due to the fact that the Fermion loop correction
can make part of the Higgs potential negative, one naturally obtains a large
equation of state(EoS) parameter in the contracting phase, which can eliminate
the anisotropy problem. After the bounce, the model can drive the universe into
the standard higgs inflation phase, which can generate nearly scale-invariant
power spectrum.
