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Antoine Bédard is a theoretical astrophysicist at the University of Warwick specializing in stellar astrophysics. His research focuses on white dwarfs, which serve as the final evolutionary stage for more than 95% of stars. These dense, inert stellar remnants cool over billions of years, allowing them to act as 'cosmic clocks' and providing valuable insights into the formation and evolution of stars and planetary systems. His current work involves the development of advanced models that describe the structure and evolution of white dwarfs, incorporating a wide array of physical theories and numerical techniques. He is particularly interested in the phenomenon of crystallization, which refers to the phase transition that leads to the stellar core freezing into a solid state and its consequent impact on the cooling process. His studies include the analysis of chemical element transport in the stellar envelope, investigating convergence effects on white dwarf evolution. Additionally, Bédard evaluates data from the Gaia satellite, analyzing hundreds of thousands of white dwarfs in the local region of the Galaxy, using atmospheric models to interpret photometric and spectroscopic observations to ascertain fundamental stellar parameters such as mass, radius, temperature, composition, and age. His research also covers binary systems of white dwarfs, contributing to important findings in stellar evolution, gravitational waves, and supernova events.
Includes General, Mechanical, Civil, Electrical, Biomedical, and Manufacturing Engineering. Most programs fall under English Band A.