activity
20242026
collaborators

6 papers

astro-ph.CO2026

A Dynamical Equilibrium Linking Nanohertz Stochastic Gravitational Wave Background to Cosmic Structure Formation

Manjia Liang, Peng Xu, Ruijun Shi +6

The stochastic gravitational wave background (SGWB) is conventionally treated as a passive relic of its astrophysical and cosmological sources, with negligible back-reaction on the…

gr-qc2025

Compact Binary Coalescence Gravitational Wave Signals Counting and Separation

Tianyu Zhao, Yue Zhou, Ruijun Shi +3

As next-generation gravitational-wave (GW) observatories approach unprecedented sensitivities, the need for robust methods to analyze increasingly complex, overlapping signals beco…

gr-qc2025

GWAI: Artificial Intelligence Platform for Enhanced Gravitational Wave Data Analysis

Tianyu Zhao, Yue Zhou, Ruijun Shi +2

Gravitational wave (GW) astronomy has opened new frontiers in understanding the cosmos, while the integration of artificial intelligence (AI) in science promises to revolutionize d…

gr-qc2025

Dawning of a New Era in Gravitational Wave Data Analysis: Unveiling Cosmic Mysteries via Artificial Intelligence -- A Systematic Review

Tianyu Zhao, Ruijun Shi, Yue Zhou +2

Gravitational wave data analysis (GWDA) faces significant challenges due to high-dimensional parameter spaces and non-Gaussian, non-stationary artifacts in the interferometer backg…

astro-ph.IM2024

Accelerating Stochastic Gravitational Wave Backgrounds Parameter Estimation in Pulsar Timing Arrays with Flow Matching

Bo Liang, Chang Liu, Tianyu Zhao +9

Pulsar timing arrays (PTAs) are essential tools for detecting the stochastic gravitational wave background (SGWB), but their analysis faces significant computational challenges. Tr…

gr-qc2024

Rapid eccentric spin-aligned binary black hole waveform generation based on deep learning

Ruijun Shi, Yue Zhou, Tianyu Zhao +2

Accurate waveform templates of binary black holes (BBHs) with eccentric orbits are essential for the detection and precise parameter estimation of gravitational waves (GWs). While…