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  <identifier identifierType="DOI">10.18453/rosdok_id00001082</identifier>
  <creators>
    <creator>
      <creatorName nameType="Personal">Lorenzen, Winfried</creatorName>
      <givenName>Winfried</givenName>
      <familyName>Lorenzen</familyName>
      <nameIdentifier nameIdentifierScheme="GND" schemeURI="http://d-nb.info/gnd/">http://d-nb.info/gnd/1029198284</nameIdentifier>
    </creator>
  </creators>
  <titles>
    <title>Phase Transitions in Hydrogen-Helium Mixtures</title>
    <title>Phasenübergänge in Wasserstoff-Helium-Mischungen</title>
  </titles>
  <publisher>Universität Rostock</publisher>
  <publicationYear>2012</publicationYear>
  <resourceType resourceTypeGeneral="Text" />
  <subjects>
    <subject xml:lang="en" schemeURI="http://dewey.info/" subjectScheme="dewey">530 Physics</subject>
  </subjects>
  <dates>
    <date dateType="Created">2012</date>
  </dates>
  <language>en</language>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="PURL">http://purl.uni-rostock.de/rosdok/id00001082</alternateIdentifier>
    <alternateIdentifier alternateIdentifierType="URN">urn:nbn:de:gbv:28-diss2012-0121-8</alternateIdentifier>
  </alternateIdentifiers>
  <descriptions>
    <description descriptionType="Abstract">Results from extensive abinitio calculations for hydrogen, helium and their mixtures at high pressures are reported. For H, special attention has been paid to the nonmetal-to-metal-transition and its accompanying first-order liquid-liquid phase transition. Furthermore, an accurate wide range EOS is calculated for He, which is of paramount interest for interior structure models of giant planets and brown dwarfs. A high pressure phase diagram of He is derived. Finally, the miscibility gap of H and He is calculated and its implication for the structure and evolution of giant planets is discussed.</description>
  </descriptions>
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