I am working on the intersection of high-energy particle physics and astrophysics. During my time in Professor Samuel Ting’s group at the Massachusetts Institute of Technology, I participated in both detector development and physics analysis for the Alpha Magnetic Spectrometer (AMS) experiment. My work contributed to several key advances: I developed a new charge reconstruction method that improved the charge resolution of AMS by more than a factor of two, supporting the collaboration’s groundbreaking results in heavy cosmic ray nuclei (published in five Physical Review Letters). I led studies on the time evolution of cosmic rays, including crucial data analysis of protons and helium nuclei, which resulted in six AMS collaboration papers on solar physics (Physical Review Letters). I also led the analysis of the origin of lithium isotopes, which was published in Physical Review Letters and selected as an Editors’ Suggestion.

Since returning to China, I have continued my interdisciplinary research in particle and astrophysics. Currently, I work on the Jiangmen Underground Neutrino Observatory (JUNO), using neutrinos to probe supernova explosion mechanisms and search for new physics. My research focuses on precision measurements of reactor neutrino oscillations and the determination of neutrino mass ordering, the first detection of the diffuse supernova neutrino background (DSNB), and the development of a supernova early warning system. I aim to contribute to major breakthroughs in neutrino physics, supernova research, and multi-messenger astronomy.

Aug. 2016 – Sep. 2018 Massachusetts Institute of Technology Ph.D.

Sep. 2012 – Jun. 2016 Xi’an Jiaotong University B.S.

May 2025 – Present Institute of High Energy Physics, Chinese Academy of Sciences, Associate Researcher

Apr. 2022 – May 2025 Massachusetts Institute of Technology, Research Scientist

Sep. 2018 – Apr. 2022 Massachusetts Institute of Technology, Postdoctoral Associate

（1） Properties of Cosmic Lithium Isotopes Measured by the Alpha Magnetic Spectrometer, Phys. Rev. Lett., 2025, 
（2） Solar Modulation of Cosmic Nuclei over a Solar Cycle: Results from the Alpha Magnetic Spectrometer, Phys. Rev. Lett., 2025, 
（3） Antiprotons and Elementary Particles over a Solar Cycle: Results from the Alpha Magnetic Spectrometer, Phys. Rev. Lett., 2025, 
（4） Properties of Cosmic Deuterons Measured by the Alpha Magnetic Spectrometer, Phys. Rev. Lett., 2024, 
（5） Temporal Structures in Positron Spectra and Charge- Sign Effects in Galactic Cosmic Rays, Phys. Rev. Lett., 2023, 
（6） Properties of Cosmic-Ray Sulfur and Determination of the Composition of Primary Cosmic-Ray Carbon, Neon, Magnesium, and Sulfur: Ten-Year Results from the Alpha Magnetic Spectrometer, Phys. Rev. Lett., 2023, 
（7） Temporal Structures in Electron Spectra and Charge Sign Effects in Galactic Cosmic Ray, Phys. Rev. Lett., 2023, 
（8） Properties of Daily Helium Fluxes, Phys. Rev. Lett., 2022, 
（9） Periodicities in the Daily Proton Fluxes from 2011 to 2019 Measured by the Alpha Magnetic Spectrometer on the International Space Station from 1 to 100 GV, Phys. Rev. Lett., 2021, 
（10） Properties of a New Group of Cosmic Nuclei: Results from the Alpha Magnetic Spectrometer on Sodium, Aluminum, and Nitrogen, Phys. Rev. Lett., 2021, 
（11） Properties of Heavy Secondary Fluorine Cosmic Rays: Results from the Alpha Magnetic Spectrometer, Phys. Rev. Lett., 2021, 
（12） The Alpha Magnetic Spectrometer (AMS) on the inter- national space station: Part II-Results from the first seven years, Physics Reports, 2021, 
（13） Properties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer, Phys. Rev. Lett., 2021, 
（14） Properties of Neon, Magnesium, and Silicon Primary Cosmic Rays Results from the Alpha Magnetic Spectrometer, Phys. Rev. Lett., 2020, 
（15） Nuclei charge measurement by the Alpha Magnetic Spectrometer silicon tracker, Nucl. Instrum. Methods Phys. Res. A, 2020.