  Since the unexpected discovery of fast radio bursts (FRBs), researchers have
proposed varied theories and models to explain these phenomena. One such model
that has recently been developed incorporates the so-called
Gertsenshtein-Zel'dovich (GZ) effect, which states that when gravitational
waves traverse a pulsar magnetosphere, a portion of the gravitational radiation
is transformed into electromagnetic (EM) radiation. The observed properties of
FRBs are consistent with the properties of this EM radiation, implying,
remarkably, that the GZ effect can account for both repeating and non-repeating
FRBs. If this model is correct, the pulsar's properties should not change over
time, and it would continue to emit both EM dipole and gravitational quadrupole
radiation for a long period of time. This article targets the gravitational
radiation produced by the pulsar mechanism and shows that several proposed
gravitational wave detectors can detect these gravitational waves. If such
detections are performed in the future from the location of FRBs, it might
validate the GZ process for FRB production and potentially rule out several
other theories of FRB generation.
