Equation of state for dark energy in<i>f</i>(<i>T</i>) gravity
Kazuharu BambaDepartment of Physics, National Tsing Hua University, Hsinchu, 300 TaiwanChao-Qiang GengDepartment of Physics, National Tsing Hua University, Hsinchu, 300 TaiwanChung-Chi LeeDepartment of Physics, National Tsing Hua University, Hsinchu, 300 TaiwanLing-Wei LuoDepartment of Physics, National Tsing Hua University, Hsinchu, 300 Taiwan
2011en
ABI
Аннотация
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.
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