对“新暴涨宇宙”模型的再研究

Further Study of the "New Inflationary Universed Model

本文对“新暴涨宇宙”模型进行了详细的近似计算．在整个计算过程中并未把“哈勃常数”Ｈ作为真正的常数．我们研究了不同阶段的慢滚落系数和扰动，发现暴涨在有效势到过极小值之前已结束．

We present in detial an approximate calculation of the 'new inflationary universe'. We do not treat 'Hubble Constant' H as a real constant in the calculation.We study the slow-roll parameters and perturbations in different periods, and find that the inflation ends a little earn6r than the minmum of the effective potential occurs.