The Properties of Hydrogen and Helium Under Extreme Conditions

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Tidal Dissipation in Stars and Giant Planets (2014, background): “However, current models indicate that a first-order phase transition, although possible in principle (McMahon et al. 2012), is not expected in Jupiter (French et al. 2012).”
Solids, liquids, and gases under high pressure (2018, background): “Searching for the metallic state in hydrogen has been the main driving force behind relentless technological developments in the high-P sciences over the decades (McMahon et al., 2012).”
AB INITIO EQUATIONS OF STATE FOR HYDROGEN (H-REOS.3) AND HELIUM (He-REOS.3) AND THEIR IMPLICATIONS FOR THE INTERIOR OF BROWN DWARFS (2014, background): “On the other hand, ab initio simulations performed for hydrogen and helium (for a recent review, see McMahon et al. (2012)) yield very good agreement with experimental data (for hydrogen, see Becker et al. (2013) and references therein).”
A perspective on conventional high-temperature superconductors at high pressure: Methods and materials (2019, background): “Pressures in the megabar range are typically found in the interior of the planets: for example, the pressure in the core of the Earth ranges from 330 to 360 GPa [14], while that in Jupiter’s core is estimated to be above 1 TPa.”