Hydrogen-helium immiscibility boundary in gas-giant planetary interiors from machine-learning molecular dynamics.

Wang X, Hamel S, Cheng B

DOI: 10.1038/s41467-026-77117-8
Published: 2026 Sep 1
Container: Nature communications
Publisher: Not recorded
Open access: yes

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Cite this work

BibTeX

@article{allodium:10.1038/s41467-026-77117-8,
  title = {Hydrogen-helium immiscibility boundary in gas-giant planetary interiors from machine-learning molecular dynamics.},
  author = {Wang X and Hamel S and Cheng B},
  year = {2026},
  journal = {Nature communications},
  doi = {10.1038/s41467-026-77117-8},
  url = {https://doi.org/10.1038/s41467-026-77117-8}
}

RIS

TY  - JOUR
TI  - Hydrogen-helium immiscibility boundary in gas-giant planetary interiors from machine-learning molecular dynamics.
AU  - Wang X
AU  - Hamel S
AU  - Cheng B
PY  - 2026
JO  - Nature communications
DO  - 10.1038/s41467-026-77117-8
UR  - https://doi.org/10.1038/s41467-026-77117-8
ER  -

APA

X, W., S, H., & B, C. (2026). Hydrogen-helium immiscibility boundary in gas-giant planetary interiors from machine-learning molecular dynamics.. Nature communications. https://doi.org/10.1038/s41467-026-77117-8

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pubmed · retrieved 2026-11-10T14:17:54.765Z