The dynamical behavior of $f(T)$ theory
Puxun Wu, Hongwei Yu

TL;DR
This paper investigates the dynamical properties of the $f(T)$ gravity theory, demonstrating its ability to produce a realistic cosmic evolution with stable and unstable phases, including a late-time accelerated expansion.
Contribution
It provides a detailed dynamical analysis of a specific $f(T)$ model, revealing its stable de Sitter attractor and evolution from radiation to matter and dark energy dominated phases.
Findings
Stable de Sitter phase identified
Universe transitions from radiation to matter to accelerated expansion
Model supports realistic cosmic evolution without dark energy
Abstract
Recently, a new model obtained from generalizing teleparallel gravity, named theory, is proposed to explain the present cosmic accelerating expansion with no need of dark energy. In this paper, we analyze the dynamical property of this theory. For a concrete power law model, we obtain that the dynamical system has a stable de Sitter phase along with an unstable radiation dominated phase and an unstable matter dominated one. We show that the Universe can evolve from a radiation dominated era to a matter dominated one, and finally enter an exponential expansion phase.
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