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Formation of ammonia–helium compounds at high pressure
Uranus and Neptune are generally assumed to have helium only in their gaseous atmospheres. Here, we report the possibility of helium being fixed in the upper mantles of these planets in the form of NH(3)–He compounds. Structure predictions reveal two energetically stable NH(3)–He compounds with stoi...
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| Publicado no: | Nat Commun |
|---|---|
| Main Authors: | , , , , , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Nature Publishing Group UK
2020
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| Assuntos: | |
| Acesso em linha: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7308345/ https://ncbi.nlm.nih.gov/pubmed/32572021 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1038/s41467-020-16835-z |
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