Finite populations of inspiralling supermassive black hole binaries plus finite observation windows introduce non-Gaussian statistics in the pulsar timing array signal that are absent from the Gaussian approximation used in current analyses.
Burke-Spolaor, S
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Finite Populations & Finite Time: The Non-Gaussianity of a Gravitational Wave Background
Finite populations of inspiralling supermassive black hole binaries plus finite observation windows introduce non-Gaussian statistics in the pulsar timing array signal that are absent from the Gaussian approximation used in current analyses.