In Einstein-scalar-Maxwell theories, charged compact binaries produce gravitational waveforms containing a leading -1 post-Newtonian dipole correction controlled by one deviation parameter b.
Charged black-hole binary evolution at second post-newtonian order
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Charged compact binaries lose energy via both gravitational and electromagnetic radiation at next-to-leading order, yielding modified orbital frequency evolution and charge-dependent stability for circular orbits.
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Inspiral gravitational waveforms from charged compact binaries with scalar hair
In Einstein-scalar-Maxwell theories, charged compact binaries produce gravitational waveforms containing a leading -1 post-Newtonian dipole correction controlled by one deviation parameter b.
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Post-Newtonian dynamics of charged compact binaries
Charged compact binaries lose energy via both gravitational and electromagnetic radiation at next-to-leading order, yielding modified orbital frequency evolution and charge-dependent stability for circular orbits.