Plane Symmetric Dark Energy Models in the Form of Wet Dark Fluid in f (R,T) Gravity

Accelerating Universe with Viscous Cosmic String in Quadratic Form of Teleparallel Gravity

“…Chaubey et al [10] has obtained a new class of Bianchi type cosmological models in ) , ( T R f gravity, while, Sahoo et al [11] investigated an axially symmetric space-time in the presence of a perfect fluid source within the frame work of ) , ( T R f gravity. Recently, Bhoyar et al [12,13], Chirde and Shekh [14,15] have investigated some cosmological models with some fluids within the frame work of ) , ( T R f gravity. Another alternative goes back to 1928 with Einstein's attempt to unify gravity and electromagnetism through the introduction of a tetrad (vierbein) field, with the concept of absolute parallelism or teleparallelism [16] known as Tele parallel Gravity (TG) or ) (T f gravity.…”

“…Particle creation in flat Friedman Robertson Walker universe in the framework of ) (T f gravity was investigated by Setare and Houndjo [22]. Chirde and Shekh [23][24][25] [27] investigated Teleparallel energy-momentum distribution of various black hole and wormhole metrics.…”

Consequences of Holographic Dark Energy Cosmological Model in Gravity

“…For a good review of the dynamics of different dark energy models, Mishra and Biswal [1] have constructed a selfconsistent system of Bianchi Type-VI 0 cosmology in five dimensions with a binary mixture of perfect fluid and dark energy where the dark energy is chosen to be either the quintessence or Chaplygin gas using solutions to the corresponding Einstein's field equations as a quadrature and observed that the equation of state parameter for dark energy is found to be consistent with the recent observations (SNe-IaSupernova with CMBR) and Galaxy Clustering Statistics. Chirde and Shekh [2][3][4] investigated interacting two-fluid viscous dark energy and magnetized dark energy cosmological models in self creation cosmology and Lyra geometry respectively. The same authors [5,6] studied plane symmetric dark energy cosmological model in the form of wet dark fluid in ƒ(R,T) gravity.…”

“…Chirde and Shekh [2][3][4] investigated interacting two-fluid viscous dark energy and magnetized dark energy cosmological models in self creation cosmology and Lyra geometry respectively. The same authors [5,6] studied plane symmetric dark energy cosmological model in the form of wet dark fluid in ƒ(R,T) gravity. Dark energy dominated Bianchi type-VI 0 cosmological model with hybrid law of expansion in ƒ(R,T) gravity investigated by Bhoyar et al [7] .…”

“…Vacuum solution in cylindrically symmetric space time in the same gravity studied by Azadi et al [14] . Bianchi type-cosmological models with bulk viscosity in ƒ(R) theory investigated by Katore and Shaikh [15] along with many authors have discussed some features of same gravity in [16][17][18][19]. Another generalization is the gravitational action includes an arbitrary function of the Ricci scalar and trace of the stress energy tensor known as ƒ(R,T) gravity.…”