We calculate the amplitude of the de Broglie gravitational waves using the standard Einstein General Relativity. We nd that these waves disappear in the limit ~ ! 0 and when their source has a large mass and volume. From the experimental point of view, the knowledge of the amplitude allows to estimate the magnitude of the eect of the wave on a sphere of test particles. We propose also to measure a very special shift angle that does not change with time.
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