Observational constraints on the equation of state of viscous fluid in f (R, T) gravity
In this paper, we investigate a cosmological model based on viscous f (R, T) gravity as a
potential alternative to dark energy. This model incorporates bulk viscosity and is analyzed …
potential alternative to dark energy. This model incorporates bulk viscosity and is analyzed …
Effect of decoupling parameters on maximum allowable mass of anisotropic stellar structure constructed by mass constraint approach in f(Q)-gravity
In the present article anisotropic solutions with vanishing complexity in the framework of f (Q)
gravity are generated. At first, the field equations in f (Q)-gravity are gravitationally …
gravity are generated. At first, the field equations in f (Q)-gravity are gravitationally …
Phase space analysis of interacting dark energy in f(T) cosmology
In this paper, we examine the interacting dark energy model in f (T) cosmology. We assume
dark energy as a perfect fluid and choose a specific cosmologically viable form f (T)= β√ T …
dark energy as a perfect fluid and choose a specific cosmologically viable form f (T)= β√ T …
Dynamics of relativistic wormholes in the presence of dark matter density profile within f (Q, T) gravity
In this paper, we study the characteristics of wormhole models in a particular gravity theory,
namely f (Q, T)= σ Q+ λ T. Here, we derived the wormhole models by using dark matter …
namely f (Q, T)= σ Q+ λ T. Here, we derived the wormhole models by using dark matter …
Analysis of cosmological tachyon and fermion model and observation data constraints
In this work, we investigate a cosmological model with the tachyon and fermion fields with
barotropic equation of state, where pressure p, energy density ρ and barotropic index γ are …
barotropic equation of state, where pressure p, energy density ρ and barotropic index γ are …
[CITATION][C] Phase space analysis of interacting dark energy in f (T) cosmology Research
M Jamil, K Yesmakhanova, D Momeni, R Myrzakulov - 2012