Conservation laws and symmetry properties of a class of higher order theories of gravity

We consider a class of fourth order theories of gravity with arbitrary matter fields arising from a diffeomorphism invariant Lagrangian density L-T = L-G + L-M, with L-G = root-g[R + h(R)] and L-M the phenomenological representation of the nongravitational fields. We derive first the generalization of the Einstein pseudotensor and the von Freud superpotential. We then show, using the arbitrariness that is always present in the choice of pseudotensor and superpotential, that we can choose these superpotentials to have the same form as those for the Hilbert Lagrangian of general relativity (GR). In particular we may introduce the Moller superpotential of GR as associated with a double-index differential conservation law. Similarly, using the Moller superpotential we prove that we can choose the Komar vector of CR to construct a conserved quantity for isolated asymptotically fiat systems. For the example R + R-2 theory we prove then, that the active mass is equal to the total energy (or inertial mass) of the system.