Scalar-tensor gravitational waves from early matter-dominated eras can contribute to the nanohertz stochastic background and remain detectable by future SKA observations.
Rapid refitting techniques for Bayesian spectral characterization of the gravitational wave background using pulsar timing arrays
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Probing Scalar-Tensor-Induced Gravitational Waves in the nHz Band: $\texttt{NANOGrav}$ and SKA
Scalar-tensor gravitational waves from early matter-dominated eras can contribute to the nanohertz stochastic background and remain detectable by future SKA observations.