Equation of state for dark energy in $f(T)$ gravity
Kazuharu Bamba, Chao-Qiang Geng, Chung-Chi Lee, Ling-Wei Luo
TL;DR
The paper investigates the dark-energy equation of state $w_{ m DE}$ within $f(T)$ gravity, showing that single-term exponential or logarithmic models cannot realize phantom-divide crossing. By constructing a combined $f(T)$ model that blends both terms, it demonstrates that $w_{ m DE}$ can cross from $>-1$ to $<-1$, a behavior favored by recent data. Using a $y_H$-formalism, the authors derive the cosmological evolution and constrain the model with SNe Ia, BAO, and CMB observations, obtaining a best-fit around $u\approx 0.83$ with a competitive $\chi^2$ compared to $\Lambda$CDM. Overall, the work suggests that torsion-based modified gravity can accommodate dynamical dark energy while remaining consistent with current cosmological measurements.
Abstract
We study the cosmological evolutions of the equation of state for dark energy $w_{\mathrm{DE}}$ in the exponential and logarithmic as well as their combination $f(T)$ theories. We show that the crossing of the phantom divide line of $w_{\mathrm{DE}} = -1$ can be realized in the combined $f(T)$ theory even though it cannot be in the exponential or logarithmic $f(T)$ theory. In particular, the crossing is from $w_{\mathrm{DE}} > -1$ to $w_{\mathrm{DE}} < -1$, in the opposite manner from $f(R)$ gravity models. We also demonstrate that this feature is favored by the recent observational data.
