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The equation of state of hydrogen, helium, and water effects interiorstructure models of giant planets significantly. We present a new equation ofstate data table, LM-REOS, generated by large scale quantum molecular dynamicssimulations for hydrogen, helium, and water in the warm dense matter regime,i.e.for megabar pressures and temperatures of several thousand Kelvin, and byadvanced chemical methods in the complementary regions. The influence ofLM-REOS on the structure of Jupiter is investigated and compared withstate-of-the-art results within a standard three-layer model consistent withastrophysical observations of Jupiter. Our new Jupiter models predict animportant impact of mixing effects of helium in hydrogen with respect to analtered compressibility and immiscibility.

Ab initio Equation of State data for hydrogen, helium, and water and the internal structure of Jupiter