郭汉英, 邹振隆
理论物理通讯. 1982, 1(2): 237-243.
In this paper, we propose a simple finite temperature λφ4 cosmological model to show that a new type singularity free cosmological model could be established by taing a series of impoftant quantum and statistical effects into consideration such as spontaneoui rymetry breaking, trace anomaly and pirtide creation, symmetry restoration at hish temperature through.phase transition and others. To begin with, the state of the universe would be a cold singu1arity.free and horizon free Beltrami-Anti de Sitter one rather than a hot one. Then associated with the,particle creatipl, the temperature would, become higher and higher and as soon. as the temperature reached a critical value, Tc a second-order phase transition would take place and the universe would transfer to a hot radiation dominated Friedmann state.