SKAO forecasts show that planned observations will improve SGWB anisotropy constraints but remain insufficient to detect the kinematic dipole even in joint PTA-astrometry analyses.
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A review of the MPM-PN approximation scheme that yields equations of motion to 4PN order and gravitational waveforms and fluxes to 4.5PN order for compact binary systems.
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Probing Kinematic Anisotropies in the Stochastic Gravitational Wave Background with the SKA
SKAO forecasts show that planned observations will improve SGWB anisotropy constraints but remain insufficient to detect the kinematic dipole even in joint PTA-astrometry analyses.
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Post-Newtonian Theory for Gravitational Waves
A review of the MPM-PN approximation scheme that yields equations of motion to 4PN order and gravitational waveforms and fluxes to 4.5PN order for compact binary systems.