Yuxiang Xu 许宇翔
My name is Yuxiang Xu. I am currently pursuing a Ph.D. at the Institute of Mechanics, Chinese Academy of Sciences. My research spans AI for Physics and Embodied AI. My current work focuses on latent world models, world action models, and vision-language models. My long-term vision is to build embodied agents that can understand the physical world, predict how it evolves, and translate multimodal perception into reliable action in complex real-world environments.
Recent News
- 2026/06 “Estimating orbital parameters of direct imaging exoplanet using neural networks” published in Physical Review Research.
- 2026/05 “Accelerating stochastic gravitational wave backgrounds parameter estimation in pulsar timing arrays with flow matching” published in Physics Letters B.
- 2026/04 The Taiji detection-pipeline study published in Science China Physics, Mechanics & Astronomy.
- 2026/04 New preprint: FluxMC, a rapid and high-fidelity inference framework for space-based gravitational-wave observations.
- 2026/01 Machine-learning-enhanced MCMC framework for EMRI parameter estimation published in Research.
- 2025/08 “Unlocking New Paths for Efficient Analysis of Gravitational Waves...” published in Chinese Physics Letters.
- 2025/07 Joined vivo AI Lab as an Assistant AI Algorithm Engineer Intern.
- 2025/05 Joined AutoLab, Westlake University as a visiting student intern.
- 2025/05 Launched the Taiji Data Challenge. Read the original preprint.
Publications
Publication details are synchronized with my Google Scholar profile and listed by year.
2026
Accelerating stochastic gravitational wave backgrounds parameter estimation in pulsar timing arrays with flow matching
Towards realistic detection pipelines of Taiji: New challenges in data analysis and high-fidelity simulations of space-based gravitational wave antenna
FluxMC: Rapid and High-Fidelity Inference for Space-Based Gravitational-Wave Observations
Toward Efficient and Accurate EMRI Parameter Estimation: A Machine Learning-Enhanced MCMC Framework
2025
Unlocking New Paths for Efficient Analysis of Gravitational Waves from Extreme-Mass-Ratio Inspirals with Machine Learning
Gravitational wave signal denoising and merger time prediction with a deep neural network
2024
Rapid parameter estimation for merging massive black hole binaries using continuous normalizing flows
Gravitational wave signal extraction against non-stationary instrumental noises with deep neural network
Rapid parameter estimation for extreme mass ratio inspirals using machine learning
Rapid parameter estimation for merging massive black hole binaries using ODE-based generative models
Contact
- Email: xuyuxiang22 [at] mails.ucas.ac.cn
- Affiliation: Institute of Mechanics, Chinese Academy of Sciences, Beijing, China.