  We investigate a bounce realization in the framework of higher order
curvature in $ f(R,T) $ modified theory of gravity. We perform a detailed
analysis of the cosmological parameters to explain the contraction phase, the
bounce phase, and the expansion phase. Furthermore, we observe a violation of
the null energy condition, instability of the model, and a singularity upon
deceleration at the bouncing point, which are the supporting results for a
bouncing cosmology. The outcome of the slow roll parameters is satisfactory to
understand the inflation era and the equation of state parameter exhibits a
ghost condensate behavior of the model near the bounce. Additionally, we
discuss the stability of the model using linear perturbations in the Hubble
parameter as well as the energy density.
