关于k本质中平坦宇宙的一个可积宇宙学模型

IF 0.2 Q4 MATHEMATICS
K. Myrzakulov, D. Kenzhalin, T. Myrzakul
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引用次数: 0

摘要

. 研究宇宙的起源和演化是现代物理学和天体物理学中有趣而实际的方向之一。本文考虑了爱因斯坦引力和k -本质理论中引力场与标量场φ以非极小方式相互作用的宇宙模型。也就是说,在作用中,在物质场的作用下,我们考虑以拉格朗日函数为本质的特殊情况。得到了所考虑模型的相应场方程。并以德西特解的形式得到了尺度因子a (t)的特解。得到了势能V (t)和标量场φ (t)的两个解,并建立了它们的图形解。本文所得到的解析解是所考虑的可积系统的解。这些解与现有的观测数据非常吻合,能够描述宇宙膨胀的现代动力学。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
On one integrable cosmological model of the flat universe in k-essence
. The study of the origin and evolution of our Universe is one of the interesting and actual directions in modern physics and astrophysics. This paper considers the cosmological model of the Universe in the Einstein's theory of gravity and k -essence, where the gravitational field interacts in a non-minimal way with the scalar field φ . That is, in action, in the role of the matter field, we consider the special case of the Lagrange function for the essence. The corresponding field equations of the considered model are obtained. Also, particular solutions for the scale factor a ( t ) were obtained in the form of de Sitter's solution. Two solutions were found, for the potential energy V ( t ) and the scalar field φ ( t ), and their graphical solutions were also built. The analytical solutions obtained in this work are solutions of the considered integrable systems. These solutions are in good agreement with the available observational data and are able to describe the modern dynamics of the expansion of the Universe.
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CiteScore
0.30
自引率
0.00%
发文量
11
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