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Τρίτη 7 Νοεμβρίου 2017

Conductivity and dissociation in liquid metallic hydrogen and implications for planetary interiors [Physics]

Liquid metallic hydrogen (LMH) is the most abundant form of condensed matter in our solar planetary structure. The electronic and thermal transport properties of this metallic fluid are of fundamental interest to understanding hydrogen's mechanism of conduction, atomic or pairing structure, as well as the key input for the magnetic...

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