Mixed fluid cosmological model in f(R, T) gravity

We construct a locally rotationally symmetric (LRS) Bianchi type-I cosmological model inf(R, T) theory of gravity when the source of gravitation is a mixture of barotropic fluid and dark energy (DE) by employing a time-varying deceleration parameter. We observe through the behavior of the state finder parameters (r, s) that our model begins from the Einstein static era and goes to ACDM era. The equation of state (EOS) parameter (omega(d)) for DE varies from the phantom (omega < -1) phase to quintessence (omega > -1) phase, which is consistent with observational results. It is found that the discussed model can reproduce the current accelerating phase of the expansion of the universe.