My work focuses on the computational challenges of high-energy processes in astroparticle physics. During my PhD at CERN (Switzerland) and KIT (Germany), I specialized in event generators and extensive air shower simulations, which led to the development of Matrix-Cascade Equations (MCEq). This open-source software is widely used to calculate atmospheric neutrino fluxes for experiments such as IceCube, KM3NeT, and Super-/Hyper-K. Over time, my research at DESY Zeuthen (Germany) shifted toward Astroparticle Theory, focusing on modeling multi-messenger emissions from Ultra-High Energy Cosmic Ray (UHECR) sources and their transport through intergalactic space. I continued exploring UHECR phenomenology and atmospheric neutrinos at the Institute for Cosmic Ray Research (ICRR) as a JSPS fellow.

Since 2021, I have been an Assistant Research Fellow at the Institute of Physics, Academia Sinica. During this time, I rejoined the IceCube Observatory in Antarctica, where I study the impact of flux systematics on data analysis. In 2024, I also became part of the Telescope Array Collaboration—an UHECR observatory in Utah, USA—focusing on reconstructing UHECR mass composition with deep neural networks and applying other machine learning techniques to UHECR data.

The High-Energy Group at the Institute of Physics, Academia Sinica focuses on theoretical and computational research in particle physics, heavy-ion physics, cosmology, and astroparticle physics. The group has five principal investigators, around ten postdoctoral researchers from different countries, and several master’s and undergraduate students. We hold regular seminars and welcome many visitors from around the world each year.