CORDIS Project
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This project investigates turbulence in protoplanetary discs, which are crucial for planet formation. By focusing on the Hall effect in magnetohydrodynamic turbulence, the project aims to provide insights into the conditions that lead to accretion and the dynamics of these cosmic structures.
The goal of this project is to obtain a global and precise description of turbulence in protoplanetary discs.Protoplanetary discs are made of gas and dust orbiting around a young star.
Among other things, we think discs are the birth place of planets.
From the lifetime of these objects, we know that protoplanetary discs are accreting, i.e. matter is slowly ``falling'' on the central star.
However, in order to explain the accretion of matter, astrophysicists have to assume that discs are turbulen…
CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS
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