The role of carbon-nanotube vibrations in the enhanced transport of confined water

ORAL

Abstract

In the last several decades, the transport of water confined in carbon nanotubes (CNTs) generated significant research interest due to an enhanced flow rate and related potential applications. Very large, classical-molecular dynamics (MD) simulations have been performed to understand the fast water flow in CNTs, but significant issues still remain open. By using density-functional-theory (DFT) MD simulations, here we initially reveal that, in the absence of any externally applied pressure, the vibrations of the CNT's carbon atoms induce directed diffusion of water confined in medium-diameter CNTs. We found that the longitudinal vibrations of the CNT induce collective diffusion of water molecules in the direction of the CNT's axis, while the in-plane CNT vibrations further enhance the diffusion of water by breaking the H-bonds between water molecules. The results provide additional insights on the mechanism of the fast water flow in CNTs.

* This work (X. Jin, D.-L. Bao, J. A. Hachtel and S.T.P.) was supported by the US Department of Energy, Office of Science, Basic Energy Sciences at Center for Nanophase Materials Sciences, Oak Ridge National Lab, as well as grant number DE-FG02-09ER46554 and McMinn Endowment at Vanderbilt University. Calculations were performed at the National Energy Research Scientific Computing Center (NERSC), a US Department of Energy Office of Science User Facility located at Lawrence Berkeley National Laboratory, operated under contract number DE-AC02-05CH11231.

Presenters

  • Xin Jin

    University of Chinese Academy of Sciences; Vanderbilt University

Authors

  • Xin Jin

    University of Chinese Academy of Sciences; Vanderbilt University

  • Deliang Bao

    Vanderbilt University, Department of Physics and Astronomy, Vanderbilt University

  • Jordan A Hachtel

    Oak Ridge National Laboratory, Center for Nanophase Materials Sciences, Oak Ridge National Laboratory

  • Sokrates T Pantelides

    Department of Physics and Astronomy, Vanderbilt University