Finch–Skea star model in f(R,T) theory of gravity

This work discusses about the existence of compact star model in context [Formula: see text] gravity with as Ricci scalar and trace energy–momentum tensor text]. The has been developed by considering spherically symmetric spacetime consisting isotropic fluid be coupling parameter. corresponding field equations are solved choosing well-known Finch–Skea ansatz [M. R. Finch J. E. F. Skea, A realistic stellar based on an Duorah Ray, Class. Quantum Gravity 6(4) (1989) 467–476]. For continuity, we elaborate boundary conditions exterior region Schwarzschild metric. unknown constants appearing solution evaluated for PSR J 1614-2230 different values constant. physical properties model, e.g. matter density, pressure, stability, etc. have discussed both analytically graphically. analysis showed that geometry compatible each other well is stable equilibrium modified gravity.