Abstract

We review potential low-frequency gravitational-wave sources, which are expected to be detected by Taiji, a Chinese space-based gravitational-wave detector, estimate the detection rates of these gravitational-wave sources and present the parameter estimation of massive black hole binaries.

DOI:10.1142/S0217751X2050075X

https://www.worldscientific.com/doi/abs/10.1142/S0217751X2050075X

International Journal of Modern Physics A（2020）