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Evolutionary Behavior of Fractional Holographic Dark Energy within $f(T)$ Teleparallel Gravity

Elangbam Chingkheinganba Meetei, S. Surendra Singh

TL;DR

The paper studies fractional holographic dark energy (FHDE) within $f(T)$ gravity using a dynamical-systems approach in a spatially flat FRW universe. By introducing dimensionless variables and constructing an autonomous system, the authors identify four critical points corresponding to radiation, matter, FHDE-dominated de Sitter, and torsion-dominated de Sitter phases; radiation and matter epochs appear as saddle points, while two late-time attractors yield accelerated expansion. The analysis, including the dependence on the fractional parameter $\alpha$, shows that FHDE with a Hubble cutoff coupled to $f(T)$ gravity can reproduce the standard cosmic sequence and provide viable late-time acceleration, with nonhyperbolic cases at $\alpha=2$ explored via phase-space trajectories. Overall, the work demonstrates that FHDE within $f(T)$ gravity offers a consistent dynamical framework capable of describing the Universe's past, present, and future evolution under a unified approach.

Abstract

We investigate the cosmological dynamics of FHDE within $f(T)$ gravity by employing the dynamical system approach in a spatially flat FRW background. By introducing appropriate dimensionless variables, the field equations are reformulated as a closed system, which allows a systematic phase-space analysis. The 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.

Evolutionary Behavior of Fractional Holographic Dark Energy within $f(T)$ Teleparallel Gravity

TL;DR

The paper studies fractional holographic dark energy (FHDE) within gravity using a dynamical-systems approach in a spatially flat FRW universe. By introducing dimensionless variables and constructing an autonomous system, the authors identify four critical points corresponding to radiation, matter, FHDE-dominated de Sitter, and torsion-dominated de Sitter phases; radiation and matter epochs appear as saddle points, while two late-time attractors yield accelerated expansion. The analysis, including the dependence on the fractional parameter , shows that FHDE with a Hubble cutoff coupled to gravity can reproduce the standard cosmic sequence and provide viable late-time acceleration, with nonhyperbolic cases at explored via phase-space trajectories. Overall, the work demonstrates that FHDE within gravity offers a consistent dynamical framework capable of describing the Universe's past, present, and future evolution under a unified approach.

Abstract

We investigate the cosmological dynamics of FHDE within gravity by employing the dynamical system approach in a spatially flat FRW background. By introducing appropriate dimensionless variables, the field equations are reformulated as a closed system, which allows a systematic phase-space analysis. The 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 gravity is capable of reproducing the standard cosmological sequence within a consistent dynamical framework.
Paper Structure (8 sections, 40 equations, 1 figure, 3 tables)

This paper contains 8 sections, 40 equations, 1 figure, 3 tables.

Figures (1)

  • Figure 1: Phase portrait diagrams for the autonomous dynamical system with $\alpha=1.5$