Kavli Affiliate: Qingjuan Yu | Summary:Pulsar timing arrays (PTAs) are anticipated to detect the stochastic gravitational wave background (GWB) from supermassive binary black holes (BBHs) as well as the gravitational waves from individual BBHs. Recently, a common process signal was reported by several PTAs. In this paper, we investigate the constraints on the BBH population […]
Continue.. Pulsar timing array detections of supermassive binary black holes: implications from the detected common process signal and beyond