Magnetized domain wall in f(R, T) theory of gravity

Fractal FRW model within domain wall

“…Many researchers are interested in the study of gravitational effects of domain walls. Recently Pawar et al [19] have investigated thick domain walls in the BD theory of gravitation, Katore and Hatkar [20] have explored Bianchi type -III and Kantowski-sachs domain wall cosmological models in f(R,T) theory of gravitation and found that curved walls are responsible for gravitational collapse of universe, Agrawal and Pawar [21] have studied Bianchi type -V space-time using magnetized domain wall in f(R,T) theory of gravitation and found that in the EM field model is isotropic whereas in the absence it becomes stiff fluid, Pradhan et al [22] have studied plane symmetric inhomogeneous bulk viscous domain walls in Lyra geometry, Patil et al [23] have obtained plane symmetric cosmological models of thick domain walls with viscous fluid coupled with electromagnetic field in the framework Lyra geometry.…”

Some Exact Bianchi Types Cosmological Models in f(R, T) Theory of Gravity

“…Bianchi types models have a vital role in the description and understanding of the early stages of evolution of the universe. In view of the observation of microwave background radiation, it is found that the universe is not isotropic [3,12,13]. Thus, the study of Bianchi types-III, V, VI 0 & VI h cosmological models is important in the sense that these models are homogeneous and anisotropic, from which the process of isotropization of the universe is studied through the passage of time.…”

Dynamical features of an anisotropic cosmological model

“…Zubair et al have analysed the stability of cylindrically symmetric objects with anisotropic fluids [28]. Agrawal and Pawar [35,36] have studied the magnetized domain wall and quark and strange quark matter in f (R, T ) gravity. There have been a good number of theoretical investigation on the f (R, T ) gravity theory in recent times in cosmology and astrophysics [37][38][39][40][41][42][43].…”