On gravitational radiation and the energy flux of matter
J. W. Maluf, F. F. Faria

TL;DR
This paper derives a continuity equation for gravitational energy-momentum within TEGR, analyzing energy fluxes in Bondi and Vaidya spacetimes, and shows that the TEGR energy definition aligns with Bondi and ADM energies.
Contribution
It demonstrates that the TEGR energy definition accurately describes Bondi and ADM energies and analyzes gravitational energy flux in specific spacetimes.
Findings
The gravitational energy flux in Bondi spacetime is expressed via the news function.
The TEGR energy matches the ADM energy under suitable conditions.
In Vaidya spacetime, energy variation is solely due to matter flux.
Abstract
A suitable derivative of Einstein's equations in the framework of the teleparallel equivalent of general relativity (TEGR) yields a continuity equation for the gravitational energy-momentum. In particular, the time derivative of the total gravitational energy is given by the sum of the total fluxes of gravitational and matter fields energy. We carry out a detailed analysis of the continuity equation in the context of Bondi and Vaidya's metrics. In the former space-time the flux of the gravitational energy is given by the well known expression in terms of the square of the news function. It is known that the energy definition in the realm of the TEGR yields the ADM (Arnowitt-Deser-Misner) energy for appropriate boundary conditions. Here we show that the same definition also describes the Bondi energy. The analysis of the continuity equation in Vaidya's space-time shows that the variation…
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