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Heat and charge transport in H(2)O at ice-giant conditions from ab initio molecular dynamics simulations
The impact of the inner structure and thermal history of planets on their observable features, such as luminosity or magnetic field, crucially depends on the poorly known heat and charge transport properties of their internal layers. The thermal and electric conductivities of different phases of wat...
| Autores principales: | , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
Nature Publishing Group UK
2020
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| Materias: | |
| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7367872/ https://www.ncbi.nlm.nih.gov/pubmed/32681002 http://dx.doi.org/10.1038/s41467-020-17275-5 |