In this paper, we study two different cases of inhomogeneous EOS of the form pd= w (t) ρ d+
w 1 f (H, t). We derive the energy density of dark fluid and dark matter component for both the …

Here in this paper we have proposed the Hamiltonian formalism of Bianchi type 1
cosmological model for different fluids including both viscous and non-viscous cases. We …

We propose a Hamiltonian formalism for a generalized Friedmann-Robertson-Walker
cosmology model in the presence of both a variable equation of state parameter w (a) and a …

Schrödinger time independent equation arises in Wheeler–DeWitt model of quantum
cosmology to develop a wave function for the corrections of cosmologies. In this work …

In this paper we have defined the effect of bulk viscosity on Quintessence model and scaler
field potential as well as on classical field. We have shown the same effect for modified …

Propomos a introdução do método de diferenças finitas como tópico a ser abordado na
disciplina de mecânica quântica de um curso de graduação em física. O método é …

We present a Chaplygin gas Friedmann-Robertson-Walker quantum cosmological model in
the presence of the cosmological constant. We apply the Schutz's variational formalism to …

We introduce in this paper a tomographic analysis of the properties of a Friedmann–
Lemaitre–Robertson–Walker (FLRW) universe with a perfect fluid. We first review previous …

In this work, we propose the quantization of a cosmological model describing the primordial
universe filled with five barotropic fluids, namely radiation, dust, vacuum, cosmic strings, and …

In this chapter we have defined the effect of bulk viscosity on Quintessence model and
scalar field potential as well as on classical field. We have shown the same effect for …