Guest–host interactions in gas clathrate hydrates under pressure

First-principles calculations were performed to determine equilibrium geometries, static equation of state parameters, the energetics and orientation of the guest molecule inside the 512 and 51262 cages, and vibrational frequencies of methane clathrate hydrate. According to our results, the progress...

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Detalles Bibliográficos
Autores: Izquierdo Ruiz, Fernando|||0000-0001-7237-4720, Otero de la Roza, Alberto|||0000-0002-4866-5816, Contreras García, Julia|||0000-0002-8947-9526, Menéndez Montes, José Manuel, Prieto Ballesteros, Olga, Recio Muñiz, José Manuel|||0000-0002-3182-7508
Tipo de recurso: artículo
Fecha de publicación:2015
País:España
Institución:Universidad de Oviedo (UNIOVI)
Repositorio:RUO. Repositorio Institucional de la Universidad de Oviedo
Idioma:inglés
OAI Identifier:oai:digibuo.uniovi.es:10651/70460
Acceso en línea:https://hdl.handle.net/10651/70460
https://dx.doi.org/10.1080/08957959.2014.996560
Access Level:acceso abierto
Palabra clave:methane clathrate hydrate
DFT calculations
EOS
vibrational modes
Descripción
Sumario:First-principles calculations were performed to determine equilibrium geometries, static equation of state parameters, the energetics and orientation of the guest molecule inside the 512 and 51262 cages, and vibrational frequencies of methane clathrate hydrate. According to our results, the progressive inclusion of one CH4 molecule in each clathrate cavity is always a stabilizing process up to saturation. The released energy is very similar for both types of cages. In agreement with the experimental observation of rotovibrational spectra in this hydrate, we calculate an energy barrier of less than 0.5 kcal/mol, indicating free rotation of methane inside the cages. The stabilizing effect of applied pressure leads to a red shift of the O–H stretching frequencies of the water molecules of around 80 cm−1 in average at 1 GPa.