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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 BambaChao-Qiang GengChung-Chi LeeLing-Wei Luo

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
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