English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Zendy Plus

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Zendy Tools

Zendy Open

The Monte Carlo simulation method of Panagiotopoulos has been used to study the fluid-fluid phase behavior of the helium-hydrogen system up to high pressures and temperatures. The influence of the attractive part of the potential has been investigated by carrying out the simulations also for the purely repulsive system. It is shown that fluid-fluid equilibrium in the helium-hydrogen system persists up to at least 700 kbar and 2500 K. The attraction causes a shift of the critical line to higher temperatures. Implications of these results for models of the Jovian planets are discussed.

physical review. b, condensed matter

Critical line of He-<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi mathvariant="normal">H</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math>up to 2500 K and the influence of attraction on fluid-fluid separation

Critical line of He-H2up to 2500 K and the influence of attraction on fluid-fluid separation