Lorentz transformation of three dimensional gravitational wave tensor
Xiaokai He, Xiaolin Liu, Zhoujian Cao

TL;DR
This paper derives the explicit Lorentz transformation for three-dimensional gravitational wave tensors, enabling the construction of waveforms from moving sources based on rest frame data, with applications to binary black hole kicks.
Contribution
It provides the first explicit Lorentz transformation formula for 3D gravitational wave tensors using a traditional tensor approach.
Findings
Derived the Lorentz transformation for gravitational wave tensors.
Enabled waveform construction for moving sources from rest waveforms.
Applied the method to binary black hole kick velocities.
Abstract
Recently there are more and more interest on the gravitational wave of moving sources. This introduces a Lorentz transformation problem of gravitational wave. Although Bondi-Metzner-Sachs (BMS) theory has in principle already included the Lorentz transformation of gravitational wave, the transformation of the three dimensional gravitational wave tensor has not been explicitly calculated before. Within four dimensional spacetime, gravitational wave have property of `boost weight zero' and `spin weight 2'. This fact makes the Lorentz transformation of gravitational wave difficult to understand. In the current paper we adopt the traditional three dimensional tensor description of gravitational wave. Such a transverse-traceless tensor describes the gravitational wave freedom directly. We derive the explicit Lorentz transformation of the gravitational wave tensor. The transformation is…
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