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

TL;DR

This paper evaluates the potential for early warning detection of precessing neutron-star black-hole mergers using upcoming gravitational-wave detectors, enabling localization seconds before merger.

Contribution

It introduces an analysis of early warning capabilities considering orbital precession effects with near-future detectors.

Findings

Sources can be localized within 100 deg^2 before 10-40 seconds of merger.

Detection is possible once per year for such sources.

Precession effects influence early warning detection performance.

Abstract

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. We find that a gravitational wave source can be localized in $100 \,\mathrm{deg^2}$ on the sky before $\sim 10$--$40 \,\mathrm{s}$ of time to merger once per year.