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Conductivity and dissociation in liquid metallic hydrogen and implications for planetary interiors

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...

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Bibliografske podrobnosti
izdano v:Proc Natl Acad Sci U S A
Main Authors: Zaghoo, Mohamed, Silvera, Isaac F.
Format: Artigo
Jezik:Inglês
Izdano: National Academy of Sciences 2017
Teme:
Online dostop:https://ncbi.nlm.nih.gov/pmc/articles/PMC5692551/
https://ncbi.nlm.nih.gov/pubmed/29078318
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1073/pnas.1707918114
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