CORDIS Project
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This project explores planet formation processes by studying dust growth and its effects on planetesimal formation and pebble accretion. Using advanced 3D simulations, it aims to enhance understanding of these mechanisms in various disk environments.
Understanding how planets form, both in and outside our solar system, is a fundamental question in astrophysics.
In recent years, a significant paradigm shift in our understanding of planet formation has emerged, which focuses on two key mechanisms: planetesimal formation by pebble concentration via streaming instability (SI) and planetary core growth through pebble accretion.The development of this new paradigm has revived interest in modeling dust growth and its role in planetesimal and planet…
KOBENHAVNS UNIVERSITET
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