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Armin Bergermann

Molecules in the deep interior of giant planets

Universität Rostock, 09. Januar 2024

https://doi.org/10.18453/rosdok_id00004725

Abstract: This study explores hydrogen, helium, nitrogen, and oxygen properties, especially under extreme conditions relevant to giant planets. Monte-Carlo simulations delve into the miscibility gap of hydrogen and helium, and predictions are made for hydrogen and water using Monte-Carlo simulations and ab-initio methods. Ab initio methods are used to understand nitrogen's equation of state and its liquid-liquid phase transition. These findings offer valuable insights into the behavior of these elements in extreme environments.

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