Phase Portraits of general f(T) Cosmology
A. Awad, W. El Hanafy, G.G.L. Nashed, Emmanuel N. Saridakis

TL;DR
This paper employs dynamical system methods to analyze the phase space of general $f(T)$ cosmology, revealing diverse evolutionary behaviors of the universe, including standard expansion, exotic phenomena, and compatibility with observational data.
Contribution
It introduces a novel approach transforming $f(T)$ cosmological equations into a one-dimensional autonomous system, simplifying phase space analysis and exploring a wide range of cosmological behaviors.
Findings
$f(T)$ cosmology can replicate the universe's observed evolution.
The phase space analysis uncovers exotic behaviors like bounces and singularities.
A new viable $f(T)$ model aligns with observational data and is free of instabilities.
Abstract
We use dynamical system methods to explore the general behaviour of cosmology. In contrast to the standard applications of dynamical analysis, we present a way to transform the equations into a one-dimensional autonomous system, taking advantage of the crucial property that the torsion scalar in flat FRW geometry is just a function of the Hubble function, thus the field equations include only up to first derivatives of it, and therefore in a general cosmological scenario every quantity is expressed only in terms of the Hubble function. The great advantage is that for one-dimensional systems it is easy to construct the phase space portraits, and thus extract information and explore in detail the features and possible behaviours of cosmology. We utilize the phase space portraits and we show that cosmology can describe the universe evolution in agreement with…
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