Non-Static Einstein-Rosen Universe in f(R, Lm) Gravitation Theory
Abstract
We investigate a non-static Einstein-Rosen spacetime within the f(R, Lm) framework, adopting f(R, Lm) = 1/2 R + Lχ m with Lm = −p. Firstly, field equations for Einstein-Rosen spacetime is attained in f(R, Lm) theory. An exact solution is obtained without using any restrictions for the constructed model. The equation of state parameter is attained for the model, and it is found that the parameter χ has a direct influence on the structure of the matter distribution and plays a decisive role in determining whether the matter exhibits exotic or ordinary characteristics. Also, we investigated the energy conditions, kinematical quantities, and the statefinder diagnostic pair for the model. Overall, the results demonstrate that matter-geometry coupling through Lm = −p can mimic cosmic acceleration in an inhomogeneous, cylindrically symmetric setting without introducing an explicit dark energy field.
Keywords
Einstein-Rosen universe, f(R, Lm) theory, energy conditions