On Extracting Physical Content from Asymptotically Flat Space-Time Metrics
C. Kozameh, E. T. Newman, G. Silva-Ortigoza

TL;DR
This paper develops a geometric framework to extract meaningful physical quantities like energy, momentum, and angular momentum from asymptotically flat space-times in general relativity, using null geodesic congruences and BMS symmetry.
Contribution
It generalizes shear-free null geodesic congruences to asymptotically shear-free ones, providing a geometric interpretation of the Bondi four-momentum and its evolution.
Findings
Defines a center of mass and spin vector with geometric meaning.
Derives a conservation law for angular momentum with flux.
Provides a kinematic interpretation of Bondi momentum in all asymptotically flat spacetimes.
Abstract
A major issue in general relativity, from its earliest days to the present, is how to extract physical information from any solution or class of solutions to the Einstein equations. Though certain information can be obtained for arbitrary solutions, e.g., via geodesic deviation, in general, because of the coordinate freedom, it is often hard or impossible to do. Most of the time information is found from special conditions, e.g., degenerate principle null vectors, weak fields close to Minkowski space (using coordinates close to Minkowski coordinates) or from solutions that have symmetries or approximate symmetries. In the present work we will be concerned with asymptotically flat space times where the approximate symmetry is the Bondi-Metzner-Sachs (BMS) group. For these spaces the Bondi four-momentum vector and its evolution, found from the Weyl tensor at infinity, describes the total…
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