Bianchi Type-V Cosmology in f(R,T) Gravity with Λ(T)
A new class of cosmological models in f (R, T) modified theories of gravity proposed by
Harko et al.(Phys. Rev. D 84: 024020, 2011), where the gravitational Lagrangian is given by …
Harko et al.(Phys. Rev. D 84: 024020, 2011), where the gravitational Lagrangian is given by …
Some anisotropic dark energy models in Bianchi type-V space-time
AK Yadav - Astrophysics and Space Science, 2011 - Springer
The paper deals with Bianchi type V Universe, which has dynamical energy density. We
consider Bianchi type V space-time, introducing three different skewness parameters along …
consider Bianchi type V space-time, introducing three different skewness parameters along …
Two-fluid scenario for dark energy models in an FRW universe-revisited
In this paper we study the evolution of the dark energy parameter within the scope of a
spatially homogeneous and isotropic Friedmann-Robertson-Walker (FRW) model filled with …
spatially homogeneous and isotropic Friedmann-Robertson-Walker (FRW) model filled with …
Bianchi type-III Dark Energy Model in f(R,T) Gravity
DRK Reddy, R Santhi Kumar… - International Journal of …, 2013 - Springer
A dark energy model with EoS parameter is investigated in f (R, T) gravity in Bianchi type-III
space-time in the presence of perfect fluid source. To obtain a determinate solution special …
space-time in the presence of perfect fluid source. To obtain a determinate solution special …
Dark energy models with anisotropic fluid in Bianchi Type-VI 0 space-time with time dependent deceleration parameter
We present two dark energy (DE) models with an anisotropic fluid in Bianchi type-VI 0 space-
time by considering time dependent deceleration parameter (DP). The equation of state …
time by considering time dependent deceleration parameter (DP). The equation of state …
Isotropic and anisotropic dark energy models
B Saha - Physics of Particles and nuclei, 2014 - Springer
In this review we discuss the evolution of the universe filled with dark energy with or without
perfect fluid. In doing so we consider a number of cosmological models, namely Bianchi type …
perfect fluid. In doing so we consider a number of cosmological models, namely Bianchi type …
LRS Bianchi-I anisotropic cosmological model with dominance of dark energy
AK Yadav, B Saha - Astrophysics and Space Science, 2012 - Springer
The present study deals with spatially homogeneous and anisotropic locally rotationally
symmetric (LRS) Bianchi type I cosmological model with dominance of dark energy. To get …
symmetric (LRS) Bianchi type I cosmological model with dominance of dark energy. To get …
An interacting and non-interacting two-fluid dark energy models in FRW universe with time dependent deceleration parameter
We study the evolution of the dark energy parameter in a spatially homogeneous and
isotropic FRW space-time filled with barotropic fluid and dark energy by considering a time …
isotropic FRW space-time filled with barotropic fluid and dark energy by considering a time …
Magnetized string cosmological models of accelerated expansion of the Universe in theory of gravity
A class of spatially homogeneous and anisotropic Bianchi-V massive string models have
been studied in the modified f (R, T)-theory of gravity proposed by Harko et al.[Phys. Rev. D …
been studied in the modified f (R, T)-theory of gravity proposed by Harko et al.[Phys. Rev. D …
Dark Energy Models in f(R, T) Theory with Variable Deceleration Parameter
In this communication we have investigated Bianchi type-II dark energy (DE) cosmological
models with and without presence of magnetic field in modified f (R, T) gravity theory as …
models with and without presence of magnetic field in modified f (R, T) gravity theory as …