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arXiv · 2408.14614

Cosmological Dynamics in Interacting Scalar-Torsion f(T,$\phi$) Gravity: Investigating Energy and Momentum Couplings

Carlos Rodriguez-Benites·Manuel Gonzalez-Espinoza·Giovanni Otalora·Manuel Alva-Morales
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Abstract

We investigate the cosmological dynamics of a homogeneous scalar field non-minimally coupled to torsion gravity, which also interacts with cold dark matter through energy and momentum transfer. The matter and radiation perfect fluids are modeled using the Sorkin-Schutz formalism. We identify scaling regimes of the field during both the radiation and matter eras. Additionally, we discovered a field-dominated scaling attractor; however, it does not exhibit accelerated expansion, making it unsuitable for describing dark energy. Nevertheless, we find two attractor solutions that do exhibit accelerated expansion: one is a quintessence-like fixed point, and the other is a de Sitter fixed point.

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Carlos Rodriguez-Benites, Manuel Gonzalez-Espinoza, Giovanni Otalora, Manuel Alva-Morales. 2024-08-26. Cosmological Dynamics in Interacting Scalar-Torsion f(T,$\phi$) Gravity: Investigating Energy and Momentum Couplings. https://doi.org/10.1103/physrevd.111.043506

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