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.
Probing non-tensorial polarizations of stochastic gravitational-wave backgrounds
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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.