Early warning of precessing neutron-star black-hole binary mergers with the near-future gravitational-wave detectors

Understand

Since gravitational and electromagnetic waves from a compact binary coalescence carry independent information about the source, the joint observation is important for understanding the physical mechanisms of the emissions.

• Rapid detection and source localization of a gravitational wave signal are crucial for the joint observation to be successful.
• For a signal with a high signal-to-noise ratio, it is even possible to detect it before the merger, which is called early warning.
• In this letter, we estimate the performances of the early warning for neutron-star black-hole binaries, considering the precession effect of a binary orbit, with the near-future detectors such as A+, AdV+, KAGRA+, and Voyager.