f(T) gravity mimicking dynamical dark energy. Background and perturbation analysis
By J. Dent, S. Dutta, Emmanuel N. Saridakis. 2010
329 citations recorded by the source corpus.
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.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/a8dab9432d27bceda5b345e14e34840cad47a58e
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In Astronomy and Astrophysics
In Nuclear and High Energy Physics
Citations in the corpus
- Solar system constraints on f(T) gravity (2012, unknown): “…Ferraro (2009), Linder (2010), Myrzakulov (2011), Yerzhanov et al (2010), Wu & Yu (2010a), Chen et al. (2011), Wu & Yu (2011a), Bamba et al. (2010), Dent et al. (2011), Zheng & Huang (2011), Bamba et al. (2011), Yang (2011), Zhang et al. (2011), Cai et al. (2011), Chattopadhyay & Debnath (2011),…”