Gauge-invariant Bardeen variables for plane waves and their relation to Cartan and Killing invariants

TL;DR

This work analyzes gravitational-wave polarization in GR using three frameworks: gauge-invariant Bardeen perturbations, Newman-Penrose curvature scalars, and the Cartan-Karlhede invariant algorithm. By extending Bardeen to flat spacetime and deriving the plane-wave metric, it shows that only the two radiative TT modes survive, with scalar and vector Bardeen variables vanishing. The Cartan-Karlhede analysis of pp-waves proves degenerate, failing to distinguish the plus and cross polarizations, while Killing invariants obtained by projecting onto background Killing vectors reproduce the Bardeen variables for plane waves, providing a geometric interpretation of polarization information. The results indicate that polarization information is carried by Killing invariants rather than Cartan invariants in this setting and motivate extensions to more complex backgrounds and modified gravity where additional degrees of freedom may emerge.

Abstract

The Newman-Penrose (NP) formalism is traditionally used to analyze the polarization content of gravitational waves, while the gauge-invariant Bardeen formalism provides a complementary, and often simpler, description based on the irreducible scalar, vector, and tensor perturbations of the metric. In this work we apply the Bardeen formalism to plane gravitational waves in Minkowski spacetime, computing all scalar, vector, and tensor gauge-invariant variables explicitly and demonstrating that only the two transverse-traceless tensor modes survive, as expected for vacuum waves in general relativity. We then compare these Bardeen variables with curvature-based invariants constructed using the linearized Cartan--Karlhede (CK) algorithm. We show that the CK invariants do not distinguish the $\oplus$ and $\times$ modes. Instead, we show that the Bardeen variables coincide with the Killing invariants obtained by projecting the metric perturbation onto the translational Killing vectors of the Minkowski background. Thus, in the plane-wave case, the physical gravitational-wave degrees of freedom are encoded in invariants generated from the Killing vector fields, rather than Cartan invariants.