Molecules in the deep interior of giant planets Bergermann, Armin , 1993- (VerfasserIn) Redmer, Ronald , 1958- (AkademischeR BetreuerIn) Baer, Roi (AkademischeR BetreuerIn) Universität Rostock (Grad-verleihende Institution) Universität Rostock Mathematisch-Naturwissenschaftliche Fakultät (Grad-verleihende Institution) Text theses Text Hochschulschrift 2024 09. Januar 2024 eng ger electronic resourceremoteComputermedienOnline-Ressourceapplication/pdf1 Online-Ressource (vii, 100 Seiten) Illustrationen, Diagramme 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.<eng> Open Access Urheberrechtsschutz 1.0 vorgelegt von Armin Bergermann Enthält Zeitschriftenartikel GutachterInnen: Ronald Redmer (Universität Rostock) ; Roi Baer (Fritz Haber Center for Molecular Dynamics, Hebrew University of Jerusalem) Dissertation Universität Rostock 2024 Kumulative Dissertation 530 530.44 530 https://purl.uni-rostock.de/rosdok/id00004725 https://doi.org/10.18453/rosdok_id00004725 https://nbn-resolving.org/urn:nbn:de:gbv:28-rosdok_id00004725-5 https://d-nb.info/1355150558/34 Molecules in the deep interior of giant planets--(DE-627)1915802601 urn:nbn:de:gbv:28-rosdok_id00004725-5 doi: 10.18453/rosdok_id00004725 oclc: 1492192651 ppn: (DE-627)191580194X