In this work, first, we study a flat Friedmann–Robertson–Walker Universe with two scalar
fields but only one potential term, which can be thought as a simple quintessence plus a K …

We investigate the phase-space structure of the quintom dark energy paradigm in the
framework of spatially flat and homogeneous universe. We have also included radiation and …

Abstract The Friedmann-Robertson-Walker (FRW) cosmology is analyzed with a general
potential V (ϕ) V(ϕ) in the scalar field inflation scenario. The Bohmian approach (a WKB-like …

Quantum cosmology with quintom dark energy model has been investigated in the present
work using symmetry analysis of the underlying physical system. In the background of the …

The multi-scalar field cosmology of the anisotropic Bianchi type-I model is used in order to
construct a family of potentials that are the best suited to model the inflation phenomenon …

In this work, we provide some simple analytical solutions to the Wheeler–DeWitt equation for
the minisuperspace applied to de Broglie–Bohm quantum cosmology for particular …

In this article, with an overview to the dynamics of the homogeneous and isotropic
cosmology for the usual and phantom scalar fields, we investigate the model of …

We construct the quintom potential of dark energy models in the framework of spatially flat
Friedmann–Robertson Walker universe in the inflationary epoch, using the Bohm like …

We derive a special scalar field potential using the anisotropic Bianchi type I cosmological
model from canonical quantum cosmology under determined conditions in the evolution to …

A flat Friedmann‐Robertson‐Walker (FRW) multiscalar field cosmology is studied with a
particular potential of the form V (ϕ, σ)= V 0 e-λ 1 ϕ-λ 2 σ, which emerges as a relation …