title: |
Molecules in the deep interior of giant planets |
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contributing persons: |
Armin Bergermann[VerfasserIn] |
 |
1354643887 |
Ronald Redmer[AkademischeR BetreuerIn] |
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136161324 |
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Universität Rostock |
Roi Baer[AkademischeR BetreuerIn] |
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Fritz Haber Center for Molecular Dynamics, Hebrew University of Jerusalem |
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contributing corporate bodies: |
Universität Rostock[Grad-verleihende Institution] |
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38329-6 |
Universität Rostock. Mathematisch-Naturwissenschaftliche Fakultät[Grad-verleihende Institution] |
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2147083-2 |
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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.
[English] |
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document type: |
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institution: |
Faculty of Mathematics and Natural Sciences |
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language: |
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subject class (DDC): |
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extent: |
1 Online-Ressource (vii, 100 Seiten)
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publication / production: |
Rostock
Rostock: Universität Rostock
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09. Januar 2024
(normalised date: 2024) |
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statement of responsibility: |
vorgelegt von Armin Bergermann |
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notes: |
Enthält Zeitschriftenartikel |
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identifiers: |
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access condition: |
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license/rights statement: |
all rights reserved This work may only be used under the terms of the German Copyright Law (Urheberrechtsgesetz). |
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RosDok id: |
rosdok_disshab_0000003216 |
created / modified: |
28.01.2025 / 29.01.2025
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metadata license: |
The metadata of this document was dedicated to the public domain (CC0 1.0 Universal Public Domain Dedication). |