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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.

Equation of state for dark energy in $f(T)$ gravity

TL;DR

The paper investigates the dark-energy equation of state within gravity, showing that single-term exponential or logarithmic models cannot realize phantom-divide crossing. By constructing a combined model that blends both terms, it demonstrates that can cross from to , a behavior favored by recent data. Using a -formalism, the authors derive the cosmological evolution and constrain the model with SNe Ia, BAO, and CMB observations, obtaining a best-fit around with a competitive compared to 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 in the exponential and logarithmic as well as their combination theories. We show that the crossing of the phantom divide line of can be realized in the combined theory even though it cannot be in the exponential or logarithmic theory. In particular, the crossing is from to , in the opposite manner from gravity models. We also demonstrate that this feature is favored by the recent observational data.

Paper Structure

This paper contains 12 sections, 49 equations, 12 figures, 1 table.

Figures (12)

  • Figure 1: $w_{\mathrm{DE}}$ as a function of the redshift $z$ for $\vert{p}\vert=0.1$ (solid line), $0.01$ (dashed line), $0.001$ (dash-dotted line) and $\Omega_{\mathrm{m}}^{(0)} = 0.26$ in the exponential $f(T)$ theory, where the left and right panels are for $p>0$ and $p<0$, respectively.
  • Figure 2: $w_{\mathrm{DE}}$ as a function of $\vert{ T/T_0 }\vert$, where the thin solid line shows $w_{\mathrm{DE}}=-1$ (cosmological constant). Legend is the same as Fig. \ref{['fig-1']}.
  • Figure 3: $\vert{ T/T_0 }\vert$ as a function of the redshift $z$ for $\vert{p}\vert=0.1$.
  • Figure 4: $\rho^{\star}_{\mathrm{DE}} \equiv \rho_{\mathrm{DE}}/\rho_{\mathrm{DE}}^{(0)}$ as a function of the redshift $z$, where the thin solid line shows $w_{\mathrm{DE}}=-1$ (cosmological constant). Legend is the same as Fig. \ref{['fig-1']}.
  • Figure 5: $\Omega_{\mathrm{DE}}$ (dashed line), $\Omega_{\mathrm{m}}$ (solid line) and $\Omega_{\mathrm{r}}$ (dash-dotted line) as functions of the redshift $z$ for $\vert{p}\vert=0.1$. Legend is the same as Fig. \ref{['fig-1']}.
  • ...and 7 more figures