Speaker
Description
Relativistic plasma astrophysics has undergone rapid development in recent years, driven by increasingly sophisticated observations and large-scale, high-fidelity numerical simulations. These advances have shed new light on a range of phenomena, including the broadband emission mechanisms of neutron star magnetospheres and the accretion flows and relativistic jets in both stellar-mass and supermassive black holes. In this talk, I will present recent progress in these areas, with particular emphasis on state-of-the-art numerical methods. I will demonstrate how simulations not only test existing theoretical models but often lead to the development of new paradigms. I will also highlight some of our group's current work on ambitious simulation campaigns aimed at addressing open questions in high-energy astrophysics.