General theory of relativity can be equivalently formulated on a flat spacetime associating a
torsion-free affine connection of non-vanishing non-metricity scalar Q. In this paper, we …

In this paper, we study the evolution of Bianchi-I spacetimes within the framework of the
Horndeski theory with G 5= const./X. The spacetimes are filled a global unidirectional …

Based on the results discussed on the invariant planes in the known literature [Universe
2022, 8, 365] for the flat FLRW space-time universe model with ideal fluid under the gravity …

Using the dynamical systems approach together with the cosmographic parameters, we
present a model-independent dynamical system formulation for cosmology in f (R) gravity …

We study anisotropic solutions for the pure gravity model with a scalar field in the Bianchi I
metric. The evolution equations have a singularity at zero value of the Ricci scalar for …

Isotropization of the magnetic universe in Horndeski theory with G3(X,ϕ) and G5(X) Page 1
Isotropization of the magnetic universe in Horndeski theory with G3(X,ϕ) and G5(X) Ruslan K …

Using the dynamical systems approach together with the cosmographic parameters, we
present a\emph {model-independent} dynamical system formulation for cosmology in $ f (R) …

We consider F (R) cosmological models with a scalar field. For the R 2 model in the spatially
flat Friedmann–Lemaître–Robertson–Walker metric, the Ricci scalar R can smoothly change …

In the Bianchi I cosmology some subclasses of the Horndeski theory allow for the non-
standard anisotropy behavior. For example, the anisotropy is damped near the initial …