Quasi-homologous evolution of relativistic stars (Q2050964)

The authors have discussed the evolutionary mechanism of the relativistic spherically symmetric spacetime who is coupled with both radiating and non-radiating matter content in a coupled modified gravity called $f(R,T)$ gravity. They have formulated the Weyl tensor with two components namely electric component and magnetic component. In case of spherical symmetric line element the magnetic component vanishes identically. Structure scalars are the terms attain by the splitting the curvature tensor orthogonaly. Further, they had used transport equation constructed from a dissipation causal theory in the dissipative scenario, which enabled them to measure the explicit temperature expressions for every model.