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arXiv 2609.18790gr-qchep-th

对称驱动的 $k$-essence 宇宙学动力学

Symmetry-Driven $k$-Essence Cosmological Dynamics

Andrés Lueiza-Colipí, Nikolaos Dimakis, Genly Leon, Andronikos Paliathanasis

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中文总结 AI 辅助

该研究通过变分对称性选取 $k$-essence 模型,利用守恒律求精确解并做动力系统分析,发现其能描述暴胀并自然过渡到物质主导期。

中文摘要 AI 辅助

我们研究了一族由场方程允许非平凡变分对称性这一要求所选取的 $k$-essence 宇宙学模型。对于拉格朗日函数为 $F(R,X,\phi)=f_{1}R+f_{2}(\phi,X)$ 的 $k$-essence 理论,其中 $f_{2}(\phi,X)=\alpha X+\beta \exp\left((n-1)\phi\right)X^{n}$,缩放对称性的存在引入了一个守恒律,我们利用该守恒律获得了一个精确的真空解。我们推广了我们的分析,并通过进行动力系统分析来研究宇宙场方程相空间的结构,既考虑不存在也考虑存在无压物质源的情况。我们采用 Hubble 归一化变量和 Poincaré 紧化,以确定模型的渐近行为,并识别所有可允许的宇宙学时期,从早期到晚期行为。我们详细讨论了每个不动点作为自由参数函数的存在性和稳定性条件,并刻画了由这个对称驱动的 $k$-essence 模型所提供的宇宙学历史的完整渐近结构。我们探讨了该模型能够描述宇宙加速的条件。我们发现,对称驱动的 $k$-essence 模型可以描述暴胀时期,并自然退出到物质主导时期,此时 $k$-essence 模拟无压物质成分。

英文摘要

We investigate a family of $k$-essence cosmological models selected by the requirement that the field equations admit a nontrivial variational symmetry. Inside this general family of theories, we concentrate on the simplest modification to quintessence, induced by power-law terms of the kinetic energy. The symmetry generator introduces a conservation law which we use to obtain an exact vacuum solution. We generalize our analysis and investigate the structure of the phase-space of the cosmological field equations by performing a dynamical systems analysis, both in the absence and the presence of a pressureless matter source. We employ Hubble-normalized variables and the Poincaré compactification, so as to determine the asymptotic behavior of the model and identify all admissible cosmological epochs, from early-time to late-time behavior. We discuss in detail the existence and stability conditions of each fixed point as functions of the free parameters, and characterize the full asymptotic structure of the cosmological history as provided by this symmetry-driven $k$-essence model. We explore the conditions under which the model can describe cosmic acceleration. We find that this $k$-essence model successfully describes the inflationary epoch with a natural exit to the matter-dominated era, with the inflaton ultimately evolving to a dark matter source.

发表机构

  • Universidad de La Frontera(拉弗龙特拉大学)
  • Universidad Católica del Norte(北天主教学会大学)
  • Durban University of Technology(德班理工大学)
  • North-West University(西北大学)
  • Universidad Católica de Temuco(特木科天主教大学)
  • National Institute for Theoretical and Computational Sciences (NITheCS)(南非国家理论与计算科学研究所)

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