Varying the inverse metric in produces three identical terms. With ,In four dimensions use the Hodge star operator to define the dual covector . Then and , so equivalently
Under an infinitesimal diffeomorphism generated by ,Insert these variations intoand integrate derivatives of by parts. Diffeomorphism invariance and arbitrariness of give the Noether identityOn the covector equation of motion , this reduces to stress-energy conservation, .
The projection is tensorial. Although a covariant derivative is not -linear in its second argument, the extra term in is proportional to , whose contraction with the normal vanishes. Thus is -linear in both arguments and defines a tensor on the hypersurface.
A hypersurface normal is locally proportional to the gradient of a defining function. The Frobenius theorem therefore impliesTaking the antisymmetric part of the formula in part i gives , henceEquivalently, torsion freedom gives because the bracket of tangent vector fields is tangent.
The affine geodesic equation givesUnit normalization implies , and decomposition of the first index givesConsequently, at the intersection point,
Choose any tangent vector and let the affinely parametrized geodesic with initial tangent start at . If is totally geodesic, then remains zero. Its initial derivative is therefore zero. Part iii, with at , givesThis holds for every tangent . Since is symmetric, the polarization identity implies
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