The electroweak phase transition in GUT inspired $SO(5)\times U(1) \times SU(3)T = T_c^{\rm EW} \sim 163,$GeV, which is very similar to the behavior in the standard model in perturbation theory. A new phase appears at higher temperatures. () and $SU(2)R \times U(1){Y’}\theta_H=\piT \sim m_{\rm KK}m_{\rm KK}$ is the Kaluza-Klein mass scale typically around 13TeV and is the Aharonov-Bohm phase along the fifth dimension. The two phases become degenerate at . As the temperature drops in the evolution of the early Universe the $SU(2)R \times U(1){Y’}SU(2)R \times U(1){Y’}SU(2)_L \times U(1)_Y$ phase becomes sizable and a first-order phase transition takes place at TeV. The amount of gravitational waves produced in this left-right phase transition is small, far below the reach of the sensitivity of Laser Interferometer Space Antenna (LISA). A detailed analysis of the phase is also given. It is shown that the boson, boson and photon, with varying from 0 to , are transformed to gauge bosons in the $SU(2)R \times U(1){Y’}$ phase. Gauge couplings and wave functions of quarks, leptons and dark fermions in the phase are determined.

生成讲解博客的中文版本

生成AI智能校验的中文版本