I specialize in high-energy astrophysics, focusing on plasma processes in magnetized environments such as magnetars, black holes, stars, and accretion flows. My work integrates theoretical frameworks with advanced simulations conducted on high-performance computing systems. Specifically, my primary research investigates the origins of plasma near neutron stars and the mechanisms behind the generation of radio and X-ray bursts during magnetospheric instabilities. Motivated by the detailed observations and advanced theories of planetary magnetospheres, including those of Earth and Jupiter, I explore fundamental plasma processes in extreme astrophysical environments. I build trustworthy non-linear models of how electromagnetic energy within stellar magnetospheres transforms into signals observable through telescopes. With expertise in scientific code development, I customize simulations to capture the intricacies of diverse astrophysical environments ensuring the highest accuracy in modeling complex plasma dynamics. Beyond my research, I am deeply committed to fostering effective communication and conflict resolution within scientific teams. I actively incorporate these communication skills into my work environment, contributing to a collaborative and inclusive scientific community.