摘要: The detection of gravitational waves from coalescences of binary compact
stars by current interferometry experiments has opened up a new era of
gravitational-wave astrophysics and cosmology. The search for stochastic
gravitational-wave background is underway by correlating signals from a pair of
detectors in the detector network formed by the LIGO, Virgo, and KAGRA. In a
previous work, we have developed a method based on spherical harmonic expansion
to calculate the overlap reduction functions of the LIGO-Virgo-KAGRA network
for a polarized stochastic gravitational-wave background. In this work, we will
apply the method to calculate the overlap reduction functions of
third-generation detectors such as a ground-based network linking the Einstein
Telescope and the Cosmic Explorer, and the LISA-Taiji joint space mission.