First spectral covariance analysis of SGWB data yields upper bounds on non-stationary correlations that translate into mass-dependent limits on high-redshift PBH merger rates.
8:Upper limits on the merger rate atz = 1as a function ofMµfor the ABH population andMc for the PBH population
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The First Upper Bound on the Non-Stationary Gravitational Wave Background and its Implication on the High Redshift Binary Black Hole Merger Rate
First spectral covariance analysis of SGWB data yields upper bounds on non-stationary correlations that translate into mass-dependent limits on high-redshift PBH merger rates.