article Open AccessTop 1% cited
Equation of state for dark energy in<i>f</i>(<i>T</i>) gravity
Journal of Cosmology and Astroparticle Physics · 2011 · Vol. 2011(01) · pp. 021–021
Kazuharu Bamba✉(Nagoya University)Chao-Qiang Geng(National Tsing Hua University)Chung-Chi Lee(National Tsing Hua University)Ling-Wei Luo(National Tsing Hua University)
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.
Cosmology and Gravitation TheoriesParticle physics theoretical and experimental studiesBlack Holes and Theoretical PhysicsDark energyEquation of stateLogarithmExponential functionDark fluidf(R) gravityCosmologyLambda-CDM model
Citations
415
FWCI
22.02
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References
56
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