分数全息暗能量在 $f(T)$ 扭动引力中的演化行为

我们采用动力学系统方法研究了 FHDE 在 $f(T)$ 引力下的宇宙动力学。通过引入合适的无量纱变量，场方程被转化为封闭系统，从而实现系统的相空间分析。 resulting system admits four critical points, including two saddle points corresponding to radiation and matter-dominated epochs, and two stable points associated with a DE-dominated phase and a de Sitter solution. The radiation- and matter-dominated critical points are found to possess a saddle character in phase space, ensuring their transient nature and enabling the cosmological evolution to naturally progress toward a stable late-time accelerated attractor. The stable critical points describe accelerated expansion with effective equations of state compatible with DE and de Sitter regimes. Overall, the analysis indicates that $f(T)$ gravity is capable of reproducing the standard cosmological sequence within a consistent dynamical framework.