At any point choose orthonormal coordinates. The antisymmetries and pair symmetry of the Riemann curvature tensor leave only independent. In these coordinates,while . Since this is a tensor identity, it follows in every coordinate system that the Ricci tensor in two dimensions satisfiesThe Einstein tensor consequently vanishes identically. Hence the two-dimensional vacuum field equation contains no local gravitational dynamics, while coupling the unmodified equation to matter would require . This is the basic degeneracy of two-dimensional general relativity.
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