On the Energy-Momentum Density of Gravitational Plane Waves
T. Dereli (Koc University), R. W. Tucker (Lancaster University)

TL;DR
This paper develops a covariant, variational framework for gravitational stress-energy, constructs a tensor analogous to electromagnetic stress-energy, and identifies energy-momentum in gravitational plane waves.
Contribution
It introduces a new covariant tensor for gravitational energy-momentum derived from a variational principle, extending Einstein's formulation.
Findings
A tensor $T^G$ is constructed from the Bel tensor and a symmetric tensor field.
Helicity-2 polarized gravitational waves carry non-zero energy and momentum.
The framework aligns gravitational stress-energy with electromagnetic analogs.
Abstract
By embedding Einstein's original formulation of GR into a broader context we show that a dynamic covariant description of gravitational stress-energy emerges naturally from a variational principle. A tensor is constructed from a contraction of the Bel tensor with a symmetric covariant second degree tensor field and has a form analogous to the stress-energy tensor of the Maxwell field in an arbitrary space-time. For plane-fronted gravitational waves helicity-2 polarised (graviton) states can be identified carrying non-zero energy and momentum.
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