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arXiv 2609.24733gr-qc

形式化 $f(R)$ 与 $f(Q)$ 引力的统一动力学系统框架

Formalizing a unified dynamical system framework for $f(R)$ and $f(Q)$ gravity

Saikat Chakraborty

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中文总结 AI 辅助

本文为 $f(R)$ 和 $f(Q)$ 引力建立统一动力学系统框架,通过三种闭合方式避免辅助变量,并揭示 $f(Q)$ 中 GR 为过去吸引子及异宿轨迹的普适性。

中文摘要 AI 辅助

超越传统的哈勃归一化框架,我们使用三组不同的无量纲变量形式化了 $f(R)$ 和重合规范 $f(Q)$ 引力的统一动力学系统表述:(1)运动学宇宙学参数,(2)暗能量状态方程参数 $w$(及其 $N=\ln a$ 导数)和物质密度丰度 $\Omega_m$,以及(3)表征理论函数形状的理论空间参数 $\{m_i\}$。我们的表述不含辅助变量,通过三种等价方式闭合:(1)指定一个理论,(2)要求特定的宇宙学演化,或(3)要求特定的暗能量状态方程演化。每种闭合策略均以显式示例说明。理论闭合方法研究了 Hu-Sawicki $f(R)$ 和 $f(Q)=-2\Lambda+Q+\beta\sqrt{-Q}$ 模型的情况,传统形式体系在这些情况下失效。从 GR 物质主导时期到晚期 de-Sitter 时期的异宿轨迹对 $f(Q)$ 是普遍的,但对 $f(R)$ 则对初始条件敏感。宇宙学参数和状态方程闭合方法比较了与 $\Lambda$CDM 运动学等价($j(z)=1$)和动力学等价($w(z)=-1$)的 $f(R)$ 和 $f(Q)$ 引力。在两种情况下,GR 作为 $f(Q)$ 引力的宇宙学过去吸引子,但对 $f(R)$ 则不然。

英文摘要

Going beyond the traditional Hubble-normalized framework, we formalize a unified dynamical system formulation for $f(R)$ and coincident gauge $f(Q)$ gravity using three distinct sets of dimensionless variables: (1) kinematical cosmographic parameters, (2) the dark energy equation of state parameter $w$ (with its $N=\ln a$ derivatives) and matter density abundance $Ω_m$, and (3) theory space parameters $\{m_i\}$ characterizing the shape of the theory function. Our formulation is free of auxiliary variables, closing via three equivalent ways: (1) specifying a theory, (2) requiring a specific cosmological evolution, or (3) requiring a specific dark energy equation of state evolution. Each closure strategy is illustrated with explicit examples. The theory closure approach studies a case of Hu-Sawicki $f(R)$ and $f(Q)=-2Λ+Q+β\sqrt{-Q}$ models, where traditional formalisms fail. A heteroclinic trajectory from a GR-matter-dominated epoch to a late-time de-Sitter epoch is general for $f(Q)$, but sensitive to initial conditions for $f(R)$. The cosmographic and equation-of-state closure approaches compare $f(R)$ and $f(Q)$ gravities kinematically equivalent to $Λ$CDM ($j(z)=1$) and dynamically equivalent to $Λ$CDM ($w(z)=-1$). In both, GR acts as a cosmological past attractor for $f(Q)$ gravity, but not for $f(R)$.

发表机构

  • Institute of Research and Development, Duy Tan University(发展研究院,岘港大学)
  • Faculty of Natural Sciences, Duy Tan University(自然科学学院,岘港大学)

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