Loading…

Temperature Study of Structure and Dynamics of Methane in Carbon Nanotubes

Molecular dynamics simulations of methane molecules inside the (15,15) carbon nanotube (CNT) are performed for the temperature range from 173 to 293 K and pressures up to 700 bar. The structural and dynamic properties of 1-site and 5-site models of methane molecules are reported. The atomic model of...

Full description

Saved in:
Bibliographic Details
Published in:Journal of physical chemistry. C 2014-06, Vol.118 (22), p.12010-12016
Main Authors: Bartuś, Katarzyna, Bródka, Aleksander
Format: Article
Language:English
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:Molecular dynamics simulations of methane molecules inside the (15,15) carbon nanotube (CNT) are performed for the temperature range from 173 to 293 K and pressures up to 700 bar. The structural and dynamic properties of 1-site and 5-site models of methane molecules are reported. The atomic model of the molecules increases density of methane in the vicinity of the nanotube wall, and the decrease of temperature increases the molecular density. The 5-site molecules from the contact layer exhibit tripod orientation with respect to the CNT. The diffusion coefficients of molecular translations along the carbon nanotube and rotational motion increase with temperature, and both decrease with pressure. Temperature dependences of the coefficients are described by the Arrhenius equation. Relatively free rotations of the 5-site molecules reduce the activation energies of translational diffusion compared to the energies for the 1-site molecules. The CNT flexibility, introduced by the reactive empirical bond order potential for interactions between carbon atoms of the nanotube, has weak impact on diffusivity of methane molecules. However, motions of the CNT atoms increase slightly the activation energies of the translational diffusion and diminish the energies of the rotational diffusion for higher pressures.
ISSN:1932-7447
1932-7455
DOI:10.1021/jp501959r