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Locally Rotationally Symmetric Bianchi Type-I Dark Energy Cosmological Models in f(T) gravity | | M. E. Rodrigues
; I. G. Salako
; M. J. S. Houndjo
; J. Tossa
; | | Date: |
13 Aug 2013 | | Abstract: | We study the locally rotational symmetry Bianchi type-I dark energy model in
the framework of $f(T)$ theory of gravity, where $T$ denotes the torsion
scalar. A viable cosmological model is undertaken and the isotropization of
this latter is checked, yielding a result that reflects the real evolution of
our universe. Moreover, still in the anisotropic optic, a more complicated
$f(T)$ model is obtained from the cosmological reconstruction scheme and the
analysis shows that the universe is more anisotropic at the beginning if the
terms of higher order in $T$ are not considered. This means that the non-linear
model should be favoured by observational data. | | Source: | arXiv, 1308.2962 | | Services: | Forum | Review | PDF | Favorites | |
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