Initial Data in General Relativity Described by Expansion, Conformal Deformation and Drift
David Maxwell

TL;DR
This paper explores an extended conformal method in general relativity, introducing new parameters like volumetric and drift momentum to better handle non-constant mean curvature solutions of Einstein's constraint equations.
Contribution
It introduces a novel parametrization of solutions to the momentum constraint, including volumetric and drift momenta, extending the conformal method beyond constant mean curvature cases.
Findings
Decomposition of momentum constraint solutions into three parameters.
Identification of three candidate methods to incorporate drift momentum.
Extension of the conformal method to include volumetric and drift momenta.
Abstract
The conformal method is a technique for finding Cauchy data in general relativity solving the Einstein constraint equations, and its parameters include a conformal class, a conformal momentum (as measured by a densitized lapse), and a mean curvature. Although the conformal method is successful in generating constant mean curvature (CMC) solutions of the constraint equations, it is unknown how well it applies in the non-CMC setting, and there have been indications that it encounters difficulties there. We are therefore motivated to investigate alternative generalizations of the CMC conformal method. Introducing a densitized lapse into the ADM Lagrangian, we find that solutions of the momentum constraint can be described in terms of three parameters. The first is conformal momentum as it appears in the standard conformal method. The second is volumetric momentum, which appears as an…
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