Investigating the microscopic (plasma-kinetic) foundations of GeV Cosmic Ray (CR) proton transport theories and their dynamic influence on stellar and galactic evolution.
Leveraging advanced computational techniques, including Particle-in-Cell (PIC) and Finite-Volume solvers, to study the evolutionary intricacies of Hydrodynamic (HD) and Magnetohydrodynamic (MHD) equations.
Exploring electron and ion acceleration mechanisms in astrophysical shocks to unravel their underlying physics.
Investigating the nonlinear evolution of astrophysical plasma instabilities across different environments.