In Extended Relativity, gravitational wave polarizations from compact binaries have relative amplitudes of tensor, vector, and scalar modes fixed by source geometry, producing specific PTA correlation patterns.
Gravitational-wave tests of general relativity with groundbased detectors and pulsar-timing arrays
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Polarization structure of gravitational waves in extended relativity
In Extended Relativity, gravitational wave polarizations from compact binaries have relative amplitudes of tensor, vector, and scalar modes fixed by source geometry, producing specific PTA correlation patterns.