f(T) gravity mimicking dynamical dark energy. Background and perturbation analysis

Details f(T) gravity mimicking dynamical dark energy. Background and perturbation analysis f(T) gravity mimicking dynamical dark energy. Background and perturbation analysis

2010-10-11

arxiv.org/abs/1010.2215v2

JCAP 1101:009,2011

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

11 pages, 12 figures, version published at JCAP

Scientific paper

10.1088/1475-7516/2011/01/009

We investigate f(T) cosmology in both the background, as well as in the perturbation level, and we present the general formalism for reconstructing the equivalent one-parameter family of f(T) models for any given dynamical dark energy scenario. Despite the completely indistinguishable background behavior, the perturbations break this degeneracy and the growth histories of all these models differ from one another. As an application we reconstruct the f(T) equivalent for quintessence, and we show that the deviation of the matter overdensity evolution is strong for small scales and weak for large scales, while it is negligible for large redshifts.

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