Combined five-PTA dataset yields posterior on SGWB power-law amplitude and index consistent with nonzero signal but below 5-sigma significance, with reconstructed angular correlations matching the Hellings-Downs prediction.
The International Pulsar Timing Array checklist for the detection of nanohertz gravitational waves,
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Under explicit auxiliary structural postulates, Generalized Trace Dynamics yields a candidate CSL-type collapse-noise two-point function with a narrow Wightman line at twice the Hubble scale.
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Stochastic gravitational-wave background search using data from five pulsar timing arrays
Combined five-PTA dataset yields posterior on SGWB power-law amplitude and index consistent with nonzero signal but below 5-sigma significance, with reconstructed angular correlations matching the Hellings-Downs prediction.
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Candidate collapse-noise correlators from Generalized Trace Dynamics: a Hubble-scale spectral line under structural assumptions
Under explicit auxiliary structural postulates, Generalized Trace Dynamics yields a candidate CSL-type collapse-noise two-point function with a narrow Wightman line at twice the Hubble scale.