Wan, YP (reprint author), Chinese Acad Sci, Inst High Energy Phys, Div Theoret Phys, POB 918-4, Beijing 100049, Peoples R China.
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.
NSFC [11121092, 11033005, 11375220, 11405069]
; CAS pilotB program
; Chinese National Youth Thousand Talents Program
; USTC start-up funding [KY2030000049]
; youth innovation promotion association project
; Outstanding young scientists project of the Chinese Academy of Sciences