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.
Prospects of constraining on the polarizations of gravitational waves from binary black holes using space- and ground- based detectors
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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.