论文标题
面对特定通货膨胀模型的壮观猜想的宜人行为
Pleasant behavior of swampland conjectures in the face of specific inflationary models
论文作者
论文摘要
最近，研究人员一直在研究各种条件作为宇宙学意义的沼泽标准。他们研究了许多具有不同滚动条件的通货膨胀模型。有时，这些猜想会被修改并导致引人入胜的点。 Swampland的猜想与慢速单场通货膨胀模型矛盾。因此，在本文中，我们将简要描述用特殊方法解决这一矛盾。我们考虑了相对于通货膨胀中的耦合函数的小参数λ，并解决了这一重要的对立面。然后，我们将根据Swampland标准讨论研究通货膨胀模型的新观点。因此，我们介绍了一些通货膨胀模型，并挑战了Swampland标准。我们根据最新可观察的数据，将宇宙学参数的允许范围指定为标量光谱指数（NS）。接下来，我们研究了新约束，以确定相应模型与Swampland猜想的兼容性或不相容性。最后，我们通过绘制一些数字来表达结果并将其与最新的观察数据进行比较。
Recently researchers have been studying various conditions as swampland criteria in cosmological implications. They have studied many inflation models with different swampland conditions. Occasionally these conjectures are modified and lead to fascinating points. The swampland conjecture is in contradiction with the slow-roll single-field inflation model. So in this paper, we will briefly describe resolving this contradiction with the special method; we consider a small parameter λ with respect to a coupling function in inflation and resolve this important antithesis. Then we will discuss a new point of view in studying inflation models according to the swampland criteria. Therefore we introduce some inflation models and challenge the swampland criteria. We specify the allowable range of cosmological parameters as the tensor-to-scalar ratio (r) the scalar spectral index (ns) according to the latest observable data. Next, we study the new constraints to determine the compatibility or incompatibility of the corresponding model with the swampland conjectures. Finally, we express the results and compare them with the latest observational data by plotting some figures.
