Taiji Program: Gravitational-Wave Sources
Wen-Hong Ruan, Zong-Kuan Guo, Rong-Gen Cai, Yuan-Zhong Zhang
TL;DR
This paper reviews potential low-frequency gravitational-wave sources detectable by the Taiji space-based detector, estimates detection rates, and discusses parameter estimation for massive black hole binaries.
Contribution
It provides a comprehensive overview of expected sources, detection prospects, and parameter estimation methods for Taiji, a new space-based gravitational-wave observatory.
Findings
Estimated detection rates for various gravitational-wave sources.
Parameter estimation accuracy for massive black hole binaries.
Identification of promising sources for Taiji detection.
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.
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