Matter under extreme conditions
modelling giant planets
Nettelmann, Sandra Nadine
1975-
aut
text
theses
Text
Hochschulschrift
gw
2009
monographic
XA-DE
2009
eng
text/html
application/pdf
Online-Ressource Ill., graph. Darst.
We calculate the core mass, metallicity and cooling curves of Jupiter, Saturn, Uranus, and Neptune and evaluate the results with respect to the hydrogen equation of state, the phase diagram of water, and immiscibility of helium in hydrogen. We conclude a likely occurrence of He sedimentation, core erosion, and inhibited convection in these planets and propose alternative structure models as improved representations of these planets.
vorgelegt von: Nadine Nettelmann
Rostock, Univ., Mathematisch-Naturwiss. Fak., Diss., 2009
520
US 8500
US 8550
US 8600
US 8650
39.53
33.09
http://rosdok.uni-rostock.de/resolve?urn=urn:nbn:de:gbv:28-diss2011-0159-8
http://rosdok.uni-rostock.de/resolve?urn=urn:nbn:de:gbv:28-diss2011-0159-8&pdf
http://nbn-resolving.de/urn:nbn:de:gbv:28-diss2011-0159-8
Matter under extreme conditions
2009
Druck-Ausgabe
(DE-627)671985795
Nettelmann, Sandra Nadine, 1975 -
urn:nbn:de:gbv:28-diss2011-0159-8
838832958
rakwb
DE-627
120123
683952226
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