Exact solutions of the Hyperextended Scalar Tensor theory with potential in the Bianchi type I model
Stephane Fay

TL;DR
This paper derives exact solutions for the Hyperextended Scalar Tensor theory with potential in Bianchi type I models, analyzing cases with power and exponential laws for the 3-volume and potential.
Contribution
It provides explicit solutions for the theory with specific functional forms, advancing understanding of anisotropic cosmological models.
Findings
Exact solutions for power-law 3-volume and potential
Exact solutions for exponential-law 3-volume and potential
Insights into anisotropic cosmological dynamics
Abstract
The Hyperextended Scalar Tensor theory with a potential is defined by three free functions: the gravitational function, the Brans-Dicke coupling function and the potential. Starting from the expression of the 3-volume and the potential as function of the proper time, we determine the exact solutions of this theory. We study two important cases corresponding to power and exponential laws for the 3-volume and the potential.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Solar and Space Plasma Dynamics
