PDF) Dynamic compression of water to conditions in ice giant interiors
Deep interior of Uranus (red) and Neptune (blue) with the heavy
Exploring Ice Giant Oceans
PDF) Superionic and metallic states of water and ammonia at giant planet conditions
Dynamic compression of water to conditions in ice giant interiors
Double superionicity in icy compounds at planetary interior
PDF) Laser-driven shock experiments on precompressed water: Implications for “icy” giant planets
Observing hot dense superionic water
Stability of high-temperature salty ice suggests electrolyte permeability in water-rich exoplanet icy mantles
QMD results for equation of state of water, from lower to higher
Dynamic Compression of Water To Conditions in Ice Giant Interiors
Electrical conductivity of water measured at 140 and 180 GPa using both
Plastic deformation of superionic water ices