Solutions in the scalar-torsion theory of gravity for the power evolution of the scalar field

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In this paper, we consider power law evolution of a scalar field in the cosmological model based on scalar-torsion gravity of the kind 𝐹(𝑇, 𝜑) = 𝐹(𝜑)𝑇. The choice of a non-minimal coupling of the scalar field with torsion of the form ∼ 𝑇𝑛/2 allows us to find an exact solution to the model that is successfully consistent with observational constraints.

Teleparallel theory of gravity, cosmological parameters

Короткий адрес: https://sciup.org/142241065

IDR: 142241065   |   DOI: 10.17238/issn2226-8812.2024.1.27-32

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