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Cosmological viable f(R,T) dark energy model: dynamics and stability · Around

2013

Cosmological viable f(R,T) dark energy model: dynamics and stability

Baffou, E. H., Kpadonou, A. V., Rodrigues, M. E. et al.

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In this paper we undertake the modified theory of gravity f(R,T) where R and T are the Ricci scalar and the trace of the energy momentum tensor, respectively.

Imposing the conservation of the energy momentum tensor, we obtain a model about what dynamics and stability are studied.
The stability is developed using the de Sitter and power-law solutions.
The results show that the model presents stability for both the de Sitter and power-law solutions.

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