Abstract
In this work, we present a class of relativistic and well-behaved solution to the Einstein’s field equations for anisotropic matter distribution. We perform our analysis by using the Buchdahl ansatz for the metric function grr. Three different classes of new exact solution are found for anisotropy factor Δ. We have analyzed our model with various physical aspects such as pressure (radial as well as transverse), energy density, anisotropy factor, mass, compactness parameter, adiabatic index γ and surface redshift. A graphical analysis of energy conditions, TOV equation and causality condition indicates the model is well behaved. The physical acceptability of the model has been verified by considering compact objects with similar mass and radii, such as 4U 1820-30, Vela X-1, PSR J1614-2230, LMC X-4, SMC X-1, 4U 1538-52, Her X-1, Cyg X-2, PSR B1913+16 and PSR J1903+327.
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