We are concerned with the precise modalities by which mathematical constructions related to energy-tensors can be adapted to a tetrad-affine setting. We show that, for fairly general gauge field theories formulated in that setting, two notions of energy tensor-the canonical tensor and the stress-energy tensor-exactly coincide with no need for tweaking. Moreover we show how both notions of energy-tensor can be naturally extended to include the gravitational field itself, represented by a couple constituted by the tetrad and a spinor connection. Then we examine the on-shell divergences of these tensors in relation to the issue of local energy-conservation in the presence of torsion.1 Indeed, a straightforward physical interpretation of the Ricci tensor in terms of energy is problematic as, for example, Schwarzschild spacetime has non-zero gravitational energy while the Ricci tensor vanishes.2 The notion of covariant differential of vector-valued forms, which has been variously present in the literature for several years, is strictly related to the Frölicher-Nijenhuis bracket [38,5,39,40,41]. In this paper we will just write down the needed coordinate expressions.