Suppression of gravitational radiation

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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References in corpus (2)

• The Escape of Gravitational Radiation from the Field of Massive Bodies
• The Emergence of Radiation from Gravitational Potential Wells: The Absence of $\omega M$ Effects

Cited by in corpus (4)

• Diffusion of the electromagnetic energy due to the backscattering off Schwarzschild geometry
• Backscattering of electromagnetic and gravitational waves off Schwarzschild geometry
• A new approach to electromagnetic wave tails on a curved spacetime
• Can Schwarzschildean gravitational fields suppress gravitational waves?