The double role of Einstein's equations: as equations of motion and as vanishing energy-momentum tensor

Diffeomorphism covariant theories with dynamical background metric, like gravity coupled to matter fields in the way expressed by Einstein-Hilbert’s action or relativistic strings described by Polyakov’s action, have on-shell' vanishing energy-momentum tensor $t_{\mu\nu}$ because $t_{\mu\nu}$ is, essentially, the Eulerian derivative associated with the dynamical background metric and thus $t_{\mu\nu}$ vanishes on-shell.’ Therefore, the equations of motion for the dynamical background metric play a double role: as equations of motion themselves and as a reflection of the fact that $t_{\mu \nu }=0$. Alternatively, the vanishing property of $t_{\mu \nu }$ can be seen as a reflection of the so-called `problem of time’ present in diffeomorphism covariant theories in the sense that $t_{\mu \nu }$ are written as linear combinations of first class constraints only.