CORDIS Project
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This project focuses on understanding the structure and evolution of white dwarfs, the remnants of stars. By developing a theoretical framework and conducting advanced simulations, it aims to improve our knowledge of white dwarf characteristics and their role in cosmic history.
The vast majority of stars will become white dwarfs at the end of the stellar life cycle.
These remnants are precise cosmic clocks owing to their well constrained cooling rates.
They provide one of the most sensitive tests of when baryonic structure formation began in the Universe.
These compact matter laboratories also unravel the mass-loss in the post-main-sequence evolution and establish critical constraints for galactic evolution models. I will design a robust theoretical framework to shed n…
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