My research focuses on the gravitational wave signals produced by core-collapse supernovae, aiming to connect theoretical models with future observational data. I specialize in gravitational-wave astronomy,
computational modeling of core-collpase supernova, analysis of turbulent hydrodynamis, signal anlysis, and neutrio transport.
Black holes are formed deep within dying massive stars and they signal a special evolution away from the canonical picture where the star explodes and leaves behind a neutron star. To probe these special evolutions and the formation pathways of black holes is a crucial link between our understanding of stellar evolution and gravitational wave astrophysics.
