Exact solution of the fiels equation of the generalized cosmological F(R,T) model

K. Yerzhanov, M. B. Abilmazhinova
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Abstract

We considered cosmological model within the framework of the generalized F(R,T) gravityin flat FLRW metric.  Earlier, an exponential solution was shown for the generalized case, which describes the inflationary stage of the evolution of the Universe. In this paper, it is shown that for the particular case of the Starobinsky model, the generalized model has, amongother things, a power-law solution that describes the dust-like stage  and  the  stage  of  radiation  dominance.It  should  be  noted  that  this  solution  was  obtained  by  the  analytical  method  as  a  solution  to  the  Euler-Lagrange  equation  for  this  model,  taking  into  account  the  functions  u,  v–  describing  the  relationship  between  the  curvature  scalar  and  the  torsion  scalar,  and  depending not only on the first, but also on the second time derivative of the scale factor. This solution is of interest, since it shows not only that this model has a solution, but also that this solution can describe the modern observable Universe for more complex forms u, v than described earlier.This solution allows other related cosmological parameters to be obtained accordingly. The paper presents the parameter for the equation of state, which describes the stage of the evolution of the Universe. Keywords:generalized cosmological model, scale factor, Starobinsky model
广义宇宙学F(R,T)模型场方程的精确解
我们在广义F(R,T)引力平面FLRW度规的框架内考虑了宇宙学模型。早先,对于描述宇宙演化暴胀阶段的广义情况,给出了一个指数解。本文证明,对于斯塔宾斯基模型的特殊情况,广义模型具有幂律解,它描述了类尘阶段和辐射优势阶段。需要注意的是,该解是用解析法作为该模型欧拉-拉格朗日方程的解得到的,考虑了描述曲率标量和扭转标量关系的函数u, v -,不仅依赖于尺度因子的第一次导数,而且依赖于尺度因子的第二次导数。这个解是有趣的,因为它不仅表明这个模型有一个解,而且这个解可以以比前面描述的更复杂的形式u, v来描述现代可观测宇宙。这个解允许得到其他相关的宇宙学参数。本文给出了描述宇宙演化阶段的状态方程的参数。关键词:广义宇宙学模型,比例因子,Starobinsky模型
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