加载中…
The problem of the vacuum energy decay is studied for both signs of the cosmological constant, through the analysis of the vacuum survival amplitude, defined in terms of the {\em conformal time}, , by ${\mathcal A}(z,z^\prime)\equiv <,z|,z^\prime>$. Transition amplitudes are computed for finite time-span, , and their {\em late time} behavior (directly related to the putative decay width of the state) as well as the transients are discussed up to first order in the coupling constant, .

生成讲解博客的中文版本

生成AI智能校验的中文版本