The Einstein constraints and differential forms
Andrzej Okolow, Jakub Szymankiewicz
TL;DR
This work recasts the vacuum Einstein constraints in terms of differential forms within the Teleparallel Equivalent of General Relativity (TEGR), replacing the spatial metric by an orthonormal coframe $\theta^I$ and the extrinsic curvature by momentum forms $r_I$. In the convenient gauge $\xi^I=0$, the TEGR constraints are shown to be equivalent to the standard Einstein constraints for the spatial metric $q$ and extrinsic curvature $K$, establishing a full equivalence between the formulations. For real-analytic spatial metrics, Bryant's theorem guarantees a local coclosed coframe, which eliminates second-order terms in the scalar constraint and reduces the system to a first-order PDE set for $(\theta^I,r_I)$. This teleparallel perspective offers a new avenue for constructing exact solutions and alternative initial-value formulations, with future work addressing extensions to smooth metrics and broader gauge choices.
Abstract
We express the vacuum Einstein constraints in terms of differential forms - the forms include one-forms constituting an orthonormal coframe of the spatial metric. We show that if the metric is real-analytic, then the constraints can be always expressed locally as a system of first order PDE's - this system is obtained by a special choice of the coframe, which reduces to zero all second order terms in the scalar constraint.
