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Bianchi type-I, type-III and Kantowski-Sachs solutions in f(T) gravity

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arxiv 1408.2689 v1 pith:DCPI3DMT submitted 2014-08-12 gr-qc

M. E. Rodrigues , A. V. Kpadonou , F. Rahaman , P. J. Oliveira , M. J. S. Houndjo This is my paper · ORCID
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keywords modelssolutionsanisotropicgravitykantowski-sachsobtaineduniversebianchi
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In the context of modified tele-parallel theory of gravity, we undertake cosmological anisotropic models and search for their solutions. Within a suitable choice of non-diagonal tetrads, the decoupled equations of motion are obtained for Bianchi-I, Bianchi-III and Kantowski-Sachs models, from which we obtain the correspondent solutions. By the way, energy density and pressures are also obtained, showing, as an important result, that our universe may live a quintessence like universe even still anisotropic models are considered.

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