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- W2892280185 abstract "The direct detection of gravitational waves crowns decades of efforts in the modelling of sources and of increasing detectors' sensitivity. With future third-generation Earth-based detectors or space-based observatories, gravitational-wave astronomy will be at its full bloom. Previously brushed-aside questions on environmental or other systematic effects in the generation and propagation of gravitational waves are now begging for a systematic treatment. Here, we study how electromagnetic and gravitational radiation is scattered by a binary system. Scattering cross-sections, resonances and the effect of an impinging wave on a gravitational-bound binary are worked out for the first time. The ratio between the scattered-wave amplitude and the incident wave can be of order $10^{-5}$ for known pulsars, bringing this into the realm of future gravitational-wave observatories. For currently realistic distribution of compact-object binaries, the interaction cross-section is too small to be of relevance." @default.
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- W2892280185 date "2018-10-01" @default.
- W2892280185 modified "2023-09-25" @default.
- W2892280185 title "Scattering of scalar, electromagnetic, and gravitational waves from binary systems" @default.
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- W2892280185 doi "https://doi.org/10.1103/physrevd.98.084001" @default.
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