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arXiv · gr-qc/9703012

Suppression of gravitational radiation

W. B. Bonnor·M. S. Piper
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Abstract

We consider a burst of quadrupole gravitational radiation in the presence of a large static mass $M$ situated at its source. Some of the radiation is back-scattered off the static field of the large mass, forming a wave tail. After the burst, the tail is a pure incoming wave, carrying energy back towards the source. We calculate this energy, and, in a numerical example, compare it with the outgoing wave energy. If $M$ is sufficiently large the incoming energy can equal the outgoing energy, indicating that the primary outgoing wave is completely suppressed.

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W. B. Bonnor, M. S. Piper. 1997-03-05. Suppression of gravitational radiation. https://doi.org/10.1088/0264-9381%2F15%2F4%2F016

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