Exact cosmological solutions of scalar-torsion gravity with a self-interacting field of the Galilean type

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The equations of cosmological dynamics for inflation models based on scalar-torsion gravity with a non-minimal connection between torsion and scalar field are considered based on a power-law parameterization of the connection between the non-minimal interaction function and the Hubble parameter. Three classes of exact solutions to the equations of cosmological dynamics are obtained, which are the basis for further analysis of the evolution of cosmological perturbations and verification of cosmological models of this type using observational data.

Torsion scalar gavity, friedman’s universe, precise cosmological solutions

Короткий адрес: https://sciup.org/142241061

IDR: 142241061   |   DOI: 10.17238/issn2226-8812.2024.1.110-115

Список литературы Exact cosmological solutions of scalar-torsion gravity with a self-interacting field of the Galilean type

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