activity
20202025
most citedThe TianQin project: current progress on science and technology

377 citations · 756 across the 15 of their papers we have counts for

collaborators

16 papers

gr-qc2025

Mapping Anisotropies in the Stochastic Gravitational-Wave Background with space detector networks

Zhi-Yuan Li, Zheng-Cheng Liang, Cong-mao Zhang +2

Future space-based gravitational-wave detectors such as TianQin, LISA, and Taiji are expected to conduct joint observations. Such a multi-detector network will provide complementar…

gr-qc2025

Inferring the stochastic gravitational-wave background from eccentric stellar-mass binary black holes with spaceborne detectors

Zheng-Cheng Liang, Zhi-Yuan Li, Yi-Ming Hu

The stochastic gravitational-wave background (SGWB) from eccentric stellar-mass binary black holes (SBBHs) holds crucial clues to their origins. For the first time, we employ a Bay…

gr-qc2024

Mapping Anisotropies in the Stochastic Gravitational-Wave Background with TianQin

Zhi-Yuan Li, Zheng-Cheng Liang, En-Kun Li +2

In the milli-Hertz frequency band, stochastic gravitational-wave background can be composed of both astronomical and cosmological sources, both can be anisotropic. Numerically depi…

astro-ph.GA2024★ 56 cited

Gravitational Wave Astronomy With TianQin

En-Kun Li, Shuai Liu, Alejandro Torres-Orjuela +50

The opening of the gravitational wave window has significantly enhanced our capacity to explore the universe's most extreme and dynamic sector. In the mHz frequency range, a divers…

gr-qc2024

Unveiling a multi-component stochastic gravitational-wave background with the TianQin + LISA network

Zheng-Cheng Liang, Zhi-Yuan Li, En-Kun Li +2

Space-borne detectors, including TianQin and Laser Interferometry Space Antenna (LISA), are tasked with simultaneously observing the Galactic foreground, astrophysical and cosmolog…

gr-qc2024

Revisiting Stochastic Gravitational-wave Background in the Strong Signal Case

Zheng-Cheng Liang, Zhi-Yuan Li, En-Kun Li +2

Weak-signal limit is often used in estimating stochastic gravitational-wave background (SGWB) intensities. This approximation fails and the signal-to-noise ratio (SNR) can be much…