Vorsitzende der Sitzung
HED and Applications
- Markus Roth (TU Darmstadt)
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Prof. Ronald Redmer (University of Rostock)21.06.17, 09:15The behaviour of warm dense matter (pressures up to the TPa region and temperatures up to several eV) is of paramount importance for understanding the interior, evolution, and magnetic field of solar and extrasolar planets. While the light elements H and He are the main components of gas giants like Jupiter, mixtures of C-N-O-H-He are relevant for Neptune-like planets, and minerals of the...Go to contribution page
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Prof. David Riley (QUB)21.06.17, 09:45The study of warm dense matter is a key part of the research programme in many and varied plasma physics laboratories around the world. The reasons for such interest are several fold. Firstly, it presents a key academic challenge. Warm dense matter is a state where partial ionisation, electron degeneracy and strong coupling exist side by side and theoretical modelling is a challenge. Secondly,...Go to contribution page
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Prof. Igor Lomonosov (IPCP RAS)21.06.17, 10:15The equation of state (EOS) is the fundamental property of matter defining its individual properties. EOS is of fundamental interest and also it is required for numerical modeling of numerous processes arising under conditions of extreme energy densities. In this report we’ll present an illustrative discussion of EOS problem for WDM. It includes methods of generation and research of...Go to contribution page