Dispersion forces stabilise ice coatings at certain gas hydrate interfaces which prevent water wetting
Gas hydrates formed in oceans and permafrost occur in vast quantities on Earth representing both a massive potential fuel source and a large threat in climate forecasts. They have been predicted to be important on other bodies in our solar systems such as Enceladus, a moon of Saturn. CO$_2$-hydrates...
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ftdatacite:10.48550/arxiv.1904.06557 2023-05-15T16:37:32+02:00 Dispersion forces stabilise ice coatings at certain gas hydrate interfaces which prevent water wetting Boström, Mathias Corkery, Robert Lima, Eduardo Malyi, Oleksandr Buhmann, Stefan Y. Persson, Clas Brevik, Iver Parsons, Drew F. Fiedler, Johannes 2019 https://dx.doi.org/10.48550/arxiv.1904.06557 https://arxiv.org/abs/1904.06557 unknown arXiv https://dx.doi.org/10.1021/acsearthspacechem.9b00019 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Earth and Planetary Astrophysics astro-ph.EP Chemical Physics physics.chem-ph FOS Physical sciences article-journal Article ScholarlyArticle Text 2019 ftdatacite https://doi.org/10.48550/arxiv.1904.06557 https://doi.org/10.1021/acsearthspacechem.9b00019 2022-03-10T16:47:14Z Gas hydrates formed in oceans and permafrost occur in vast quantities on Earth representing both a massive potential fuel source and a large threat in climate forecasts. They have been predicted to be important on other bodies in our solar systems such as Enceladus, a moon of Saturn. CO$_2$-hydrates likely drive the massive gas-rich water plumes seen and sampled by the spacecraft Cassini, and the source of these hydrates is thought to be due to buoyant gas hydrate particles. Dispersion forces cause gas hydrates to be coated in a 3-4 nm thick film of ice, or to contact water directly, depending on which gas they contain. These films are shown to significantly alter the properties of the gas hydrate clusters, for example, whether they float or sink. It is also expected to influence gas hydrate growth and gas leakage. Article in Journal/Newspaper Ice permafrost DataCite Metadata Store (German National Library of Science and Technology) |
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Earth and Planetary Astrophysics astro-ph.EP Chemical Physics physics.chem-ph FOS Physical sciences |
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Earth and Planetary Astrophysics astro-ph.EP Chemical Physics physics.chem-ph FOS Physical sciences Boström, Mathias Corkery, Robert Lima, Eduardo Malyi, Oleksandr Buhmann, Stefan Y. Persson, Clas Brevik, Iver Parsons, Drew F. Fiedler, Johannes Dispersion forces stabilise ice coatings at certain gas hydrate interfaces which prevent water wetting |
topic_facet |
Earth and Planetary Astrophysics astro-ph.EP Chemical Physics physics.chem-ph FOS Physical sciences |
description |
Gas hydrates formed in oceans and permafrost occur in vast quantities on Earth representing both a massive potential fuel source and a large threat in climate forecasts. They have been predicted to be important on other bodies in our solar systems such as Enceladus, a moon of Saturn. CO$_2$-hydrates likely drive the massive gas-rich water plumes seen and sampled by the spacecraft Cassini, and the source of these hydrates is thought to be due to buoyant gas hydrate particles. Dispersion forces cause gas hydrates to be coated in a 3-4 nm thick film of ice, or to contact water directly, depending on which gas they contain. These films are shown to significantly alter the properties of the gas hydrate clusters, for example, whether they float or sink. It is also expected to influence gas hydrate growth and gas leakage. |
format |
Article in Journal/Newspaper |
author |
Boström, Mathias Corkery, Robert Lima, Eduardo Malyi, Oleksandr Buhmann, Stefan Y. Persson, Clas Brevik, Iver Parsons, Drew F. Fiedler, Johannes |
author_facet |
Boström, Mathias Corkery, Robert Lima, Eduardo Malyi, Oleksandr Buhmann, Stefan Y. Persson, Clas Brevik, Iver Parsons, Drew F. Fiedler, Johannes |
author_sort |
Boström, Mathias |
title |
Dispersion forces stabilise ice coatings at certain gas hydrate interfaces which prevent water wetting |
title_short |
Dispersion forces stabilise ice coatings at certain gas hydrate interfaces which prevent water wetting |
title_full |
Dispersion forces stabilise ice coatings at certain gas hydrate interfaces which prevent water wetting |
title_fullStr |
Dispersion forces stabilise ice coatings at certain gas hydrate interfaces which prevent water wetting |
title_full_unstemmed |
Dispersion forces stabilise ice coatings at certain gas hydrate interfaces which prevent water wetting |
title_sort |
dispersion forces stabilise ice coatings at certain gas hydrate interfaces which prevent water wetting |
publisher |
arXiv |
publishDate |
2019 |
url |
https://dx.doi.org/10.48550/arxiv.1904.06557 https://arxiv.org/abs/1904.06557 |
genre |
Ice permafrost |
genre_facet |
Ice permafrost |
op_relation |
https://dx.doi.org/10.1021/acsearthspacechem.9b00019 |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.1904.06557 https://doi.org/10.1021/acsearthspacechem.9b00019 |
_version_ |
1766027821164003328 |