activity
20242026
collaborators

6 papers

gr-qc2026

Detectability to extreme mass ratio inspirals with alternative space-based detector networks

Chao Zhang, Gang Wang

Extreme mass ratio inspirals (EMRIs) are among the primary targets for space-based gravitational-wave (GW) detectors, providing valuable opportunities to study stellar-mass compact…

gr-qc2026

Correlation and Data-Analysis Distinctiveness of Time-Delay Interferometry Configurations

Gang Wang

Time-Delay Interferometry (TDI) is essential for space-based gravitational wave (GW) missions, as it suppresses laser frequency noise and achieve the required sensitivity. Beyond t…

gr-qc2026

Time delay interferometry with minimal null frequencies and shortened time span

Gang Wang

Time-delay interferometry (TDI) is essential for suppressing laser frequency noise in space-based gravitational wave (GW) observatories such as LISA. However, current second-genera…

gr-qc2025

Detectability of massive binary black holes with sub-mHz gravitational wave missions

Renjie Wang, Yumeng Xu, Gang Wang +2

Beyond LISA, proposed space-based gravitational wave (GW) missions aim to explore the sub-millihertz to microhertz frequency band, with one key objective being the detection of mas…

gr-qc2025

Alternative LISA-TAIJI networks: Detectability of the Parity Violation in Stochastic Gravitational Wave Background

Ju Chen, Chang Liu, Yun-Long Zhang +1

The detection of parity violation in the isotropic stochastic gravitational wave background (SGWB) will serve a crucial probe for new physics, particularly in parity-violating theo…

gr-qc2024

Enhancing noise characterization with robust time delay interferometry combination

Gang Wang

Time delay interferometry (TDI) is essential for suppressing laser frequency noise and achieving the targeted sensitivity for space-borne gravitational wave (GW) missions. In Paper…