Radiating Isotropic Homogeneous f(R,G) Gravity Model with Quark and Strange Quark Matter

Abstract

Present analysis devoted to the dynamical investigation of radiating quark and strange quark matter in the framework of f(R, G) theory of gravity towards spatially homogeneous isotropic Friedman-Robertson-Walker line element filled with isotropic fluid. We govern the features of the derived cosmological model by considering the well known relation between Hubble parameter H and scale factor. Some kinematical and physical parameters for quark and strange quark matter towards isotropic model is discussed in detail.