In this work, we investigate the viable bouncing cosmological solutions in the framework of f ( Q, L m ) gravity, which incorporates the coupling between the non-metricity scalar ( Q ) and the matter-Lagrangian ( L m ). We take into consideration a Bianchi type-I spacetime with an isotropic matter distribution to examine the implications of this framework on the dynamics of the early cosmos. Two different functional versions of the f ( Q, L m ) Lagrangian are being studied and relevant modified