Baryon asymmetry via non-thermal leptogenesis is explained in the framework of the standard Coleman-Weinberg inflationary model. The CP-violation asymmetry factor arises from the out-of-equilibrium decays of heavy right-handed neutrinos in supersymmetric SO(10) GUT models. All quantities of interest are computed in terms of the two parameters of the inflationary potential, namely the vacuum expectation value of the inflaton, $M,$ and the amplitude $A$. For successful baryogenesis we obtain analytical expressions relating $A$ to $M,$ and also the reheating temperature after inflation as well as the mass of the inflaton to $M$. Assuming typical values of CP-violation asymmetry obtained in concrete supersymmetric $SO\left(10\right)$ unified models, we show graphically all three quantities of interest versus $M$. Interestingly enough, we obtain for ($A,M$) numerical values comparable to the ones previously obtained in the slow-roll approximation of inflationary dynamics upon comparison with CMB data, such as amplitude of scalar perturbations and spectral index. Proton decay is also briefly discussed. Our results may be of interest to model builders.

通过非热瘦发生的重子不对称性在标准Coleman-Weinberg膨胀模型的框架中得到解释。CP违反不对称因素是由超对称SO（10）GUT模型中右手重中微子的失衡衰减引起的。所有感兴趣的量都是根据两个潜在的通胀潜力参数来计算的，即充气子的真空期望值，$\mathrm{中号}，$ 和振幅 $\mathrm{一种}$。对于成功的重生成，我们获得与$\mathrm{一种}$ 至 $\mathrm{中号}，$ 以及充气后的再加热温度以及充气到 $\mathrm{中号}$。假定混凝土超对称中获得的CP违反不对称性的典型值$\mathrm{小号}Ø（10）$ 统一模型，我们以图形方式显示了所有三个兴趣量与 $\mathrm{中号}$。有趣的是，我们获得了$\mathrm{一种}，\mathrm{中号}$）的数值可与先前通过与CMB数据进行比较而得出的充气动力学的慢滚近似法所获得的数值进行比较，例如标量摄动的幅度和光谱指数。质子衰减也作了简要讨论。我们的结果可能对模型构建者感兴趣。