Open Bachelor & Master Projects
Project offers are open throughout the whole year. The projects give you an impression on the spectrum of our work for which we invite you to productively contribute. If you need more information or want to learn about latest opportunities, please do not hesitate to drop me an Email.
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Related to the general field of the theory of planet formation, the thesis addresses the stability of accretion disks with respect to a baroclinic instability.
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Magnetorotational turbulence plays an important role in the formation of planets. It is diffusing small grains and concentrating larger objects in turbulent features.
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Recent numerical simulations show that large, Ceres sized planetesimals might form very rapidly in protoplanetary disks. In this work we want to explore the consequences of these findings on the formation of (extrasolar) giant planets.
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