The possibility of linking inflation and late cosmic accelerated expansion using the α-
attractor models has received increasing attention due to their physical motivation. In the …

We consider a variety of quintessence scalar field models in a homogeneous and isotropic
geometry of the Universe with zero spatial curvature aiming to provide stringent constraints …

Dark energy models with tracker properties have gained attention due to the large range of
initial conditions leading to the current value of the dark energy density parameter. A well …

We study the primordial perturbations and reheating process in the models where the Gauss–
Bonnet (GB) term is nonminimally coupled to the canonical and noncanonical (DBI and …

We perform in this work an analysis of the background dynamics for α-attractor models in the
context of loop quantum cosmology. Particular attention is given to the determination of the …

In this paper, we study the model of the late universe with the homogeneous, isotropic and
flat Friedmann–Robertson–Walker metric, where the source of the gravitational field is …

We systematically study the preinflationary dynamics of the spatially flat Friedmann-Lemaitre-
Robertson-Walker universe filled with a single scalar field that has the generalized α …

By starting with a two-fields model in which the fields and their derivatives are nonminimally
coupled to gravity, and then by using a conformal gauge, we obtain a model in which the …

The cosmological models exhibiting tracker properties have great significance in the context
of dark energy as they can reach the present value of dark energy density from a wide range …

The α-attractor inflationary models are nowadays favored by CMB Planck observations.
Their similarity with canonical quintessence models motivates the exploration of a common …