Abstract
In this paper we explore \(f(T, \mathcal{T})\), where \(T\) and \(\mathcal {T}\) denote the torsion scalar and the trace of the energy-momentum tensor respectively. We impose the covariant conservation to the energy-momentum tensor and obtain a cosmological \(f(T, \mathcal{T})\) respectively. We impose the covariant conservation to the energy-momentum tensor and obtain a cosmological \(f(T, \mathcal{T})\) model. Then, we study the stability of the obtained model for power-law and de Sitter solutions and our result show that the model can be stable for some values of the input parameters, for both power-law and de Sitter solutions.
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The authors thank IMSP for hospitality during the elaboration of this work.
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Ganiou, M.G., Salako, I.G., Houndjo, M.J.S. et al. \(f(T,\mathcal{T})\) cosmological models in phase space. Astrophys Space Sci 361, 57 (2016). https://doi.org/10.1007/s10509-015-2644-5
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DOI: https://doi.org/10.1007/s10509-015-2644-5