Guest Partitioning in Carbon Monoxide Hydrate by Raman Spectroscopy
Source abstract
Abstract
Gas hydrates are inclusion compounds composed of a H-bonded water network forming cages, inside of which gaseous (guest) molecules are encapsulated. Depending on the nature and partitioning of the guest molecules, various types of clathrate structures may be formed. In this work we have elucidated the guest partitioning of the CO hydrate, using high-resolution Raman microspectroscopy, and investigated the impact of pressure–temperature ( P – T ) conditions on this partitioning. For the first time, vibrational signatures of CO molecules encapsulated in a large cage and small cage are identified. It is also shown that the large cages of the CO hydrate have the ability to easily catch or release CO guest molecules, while the small cages remain singly occupied. Moreover, the study of the P – T dependence of the Raman signature demonstrates not only the CO stretching frequency dependence with the cage filling but also the tuning effect of the cage filling by the P – T conditions of treatment.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Methane Hydrates and Related Phenomena · Hydrocarbon exploration and reservoir analysis · Astro and Planetary Science
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Groupe Spectroscopie Moléculaire - Institut des Sciences Moléculaires, UMR 5255 CNRS-Univ. Bordeaux, 351 cours de la Libération, Talence F-33404 Cedex, France
Laboratoire Léon Brillouin, UMR 12 CEA-CNRS − Bât. 563 CEA Saclay, Gif-Sur-Yvette 91191 Cedex, France
Funding
Agence Nationale de la Recherche
References (29)
Show source-provided references
1. 10.1021/ie50296a01010.1021/ie50296a010 ↗
2. Sloan E. D. · 2008
3. 10.1016/0019-1035(87)90075-310.1016/0019-1035(87)90075-3 ↗
4. 10.1126/science.113351910.1126/science.1133519 ↗
5. 10.1038/nature0815310.1038/nature08153 ↗
6. 10.1002/recl.1960079060610.1002/recl.19600790606 ↗
7. 10.1002/recl.1965084081510.1002/recl.19650840815 ↗
8. 10.1073/pnas.47.11.179810.1073/pnas.47.11.1798 ↗
9. Miller, S. L.InIces in the solar system;Klinger, J.; Benest, D.; Dollfus, A.; Smoluchowski, R., Eds;Springer:Netherlands, 1985; pp59–79.
10. 10.1086/15799210.1086/157992 ↗
11. 10.1038/328418a010.1038/328418a0 ↗
12. 10.1086/19105010.1086/191050 ↗
13. 10.1007/BF0113128310.1007/BF01131283 ↗
14. 10.1038/ncomms512810.1038/ncomms5128 ↗
15. 10.1016/j.icarus.2010.12.00410.1016/j.icarus.2010.12.004 ↗
16. 10.1021/jp970768e10.1021/jp970768e ↗
17. Chazallon B. · 2017 · 1
18. 10.1002/aic.1052610.1002/aic.10526 ↗
19. 10.1021/ie901820u10.1021/ie901820u ↗
20. Le Bail, A.InAccuracy in Powder Diffraction II: Proceedings of the International Conference May 26–29;Prince, E.; Stalick, J. K., Eds.NIST Special Publication, 1992; Vol.846, pp142–153.
21. Rodriguez-Carvajal, J.InFULLPROF: a Program for Rietveld Refinement and Pattern Matching Analysis. Proceeding of the satellite meeting on powder diffraction of the XV congress of the IUCr, Toulouse, France, 1990.
22. 10.1021/je500613y10.1021/je500613y ↗
23. 10.1021/jp013644h10.1021/jp013644h ↗
24. 10.1140/epje/i2003-10026-610.1140/epje/i2003-10026-6 ↗
25. 10.1021/je980152y10.1021/je980152y ↗
26. 10.1023/A:100796021769110.1023/A:1007960217691 ↗
27. 10.1063/1.148086110.1063/1.1480861 ↗
28. 10.1002/ange.20070025010.1002/ange.200700250 ↗
29. 10.1021/acs.jpcc.6b0652410.1021/acs.jpcc.6b06524 ↗