摘要: The coalescences of massive black hole binaries (MBHBs) are one of the main
targets of space-based gravitational wave observatories. Such gravitational
wave sources are expected to be accompanied by electromagnetic emission. Low
latency time of gravitational wave searches and accurate sky localization are
keys in triggering successful follow-up observations on the electromagnetic
counterparts. Here we present a deep learning method for the first time to
rapidly search for MBHB signals in the strain data. Our model is capable to
process 1-year of data in just several seconds, identifying all MBHB
coalescences with no false alarms. We test the performance of our model on the
simulated data from the LISA data challenge. We demonstrate that the model
shows a robust resistance for a wide range of generalization for MBHB signals.
This method is supposed to be an effective approach, which combined the
advances of artificial intelligence to open a new pathway for space-based
gravitational wave observations.