Local freedom in the gravitational field

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Abstract
In a cosmological context, the electric and magnetic parts of the Weyl tensor, and , represent the locally free curvature, i.e. they are not pointwise determined by the matter fields. By performing a complete covariant decomposition of and , 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 symmetrized trace-free spatial derivatives of and together with their spatial curls. These parts of the derivatives are shown to be crucial for the existence of gravitational waves.

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