CORDIS Project
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This project aims to enhance our understanding of accretion disks around celestial bodies by integrating magnetic fields into their models. It seeks to develop a new theoretical framework that accounts for magnetized turbulence and non-thermal radiation, addressing key astrophysical questions about the formation and ev…
Most celestial bodies, ranging from planets to stars to black holes, gain mass during their lives by gravitationally attracting matter from their environments.
This accretion process takes place via a disk-like structure around the gravitating object.
Understanding the physical processes that determine the rate at which matter accretes and energy is radiated in these disks is vital for unraveling the formation, evolution, and fate of almost every type of object in the Universe.
Despite the fact…
KOBENHAVNS UNIVERSITET
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