Many models of dark energy have been proposed to describe the universe since the beginning of the Big Bang. In this study, we present a new model of agegraphic dark energy based on the three generalized uncertainty principles KMM (Kempf, Mangan, Mann), Nouicer and $GU{P}^{*}$ (higher orders generalized uncertainty principle). Using the obtained relations from three types of Generalized Uncertainty Principle (GU P), in the form of three scenarios (Emergent, Intermediate, Logamediate), we consider three different eras of the universe evolution. Also, we describe the evolution and expansion of the universe in each subsection. We will plot the obtained relations in these models for better comparatione.

自大爆炸开始以来，已经提出了许多暗能量模型来描述宇宙。在这项研究中，我们基于三个广义不确定性原理KMM（Kempf、Mangan、Mann）、Nouicer 和$GüP^{*}$（高阶广义不确定性原理）。使用从三种类型的广义不确定性原理 ( GU P ) 获得的关系，以三种场景（紧急、中间、对数中间）的形式，我们考虑宇宙演化的三个不同时代。此外，我们在每个小节中描述了宇宙的演化和膨胀。我们将绘制这些模型中获得的关系以便更好地进行比较。