In this paper, we derive some new exact solutions of static wormholes in f (R) gravity supported by the matter possesses Lorentizian density distribution of a particle-like gravitational source. We derive the wormhole's solutions in two possible schemes for a given Lorentzian distribution: assuming an astrophysically viable F (R) function such as a power-law form and discuss several solutions corresponding to different values of the exponent ( here F = df dR ). In the second scheme, we consider particular form of two shape functions and have reconstructed f(R) in both cases. We have discussed all the solutions with graphical point of view.