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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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| Publicado no: | Proc Natl Acad Sci U S A |
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| Main Authors: | , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
National Academy of Sciences
2017
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| Assuntos: | |
| Acesso em linha: | 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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