In a cosmological context, the electric and magnetic parts of the Weyl tensor, E_{ ab} and H_{ ab}, represent the locally free curvature - i.e. they are not pointwise determined by the matter fields. By performing a complete covariant decomposition of the derivatives of E_{ ab} and H_{ ab}, we show that the parts of the derivative of the curvature which are locally free (i.e. not pointwise determined by the matter via the Bianchi identities) are exactly the symmetrised trace-free spatial derivatives of E_{ ab} and H_{ ab} together with their spatial curls. These parts of the derivatives are shown to be crucial for the existence of gravitational waves.
Categories: gr-qc