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      Quantum Monte Carlo simulations of Arn–CO2 clusters

      The Journal of Chemical Physics
      AIP Publishing

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          Abstract

          Potential-energy functions for CO2–Arn clusters are constructed using the pairwise-additive approximation from the Ar–Ar potential of Aziz [J. Chem. Phys. 99, 4518 (1993)] and three different CO2–Ar potentials which have been reported recently. These are used to find minimum-energy structures and to carry out rigid-body diffusion Monte Carlo simulations of the ground vibrational state for CO2–Arn clusters with n up to 30, as well as the first excited state for n=1. From these results, the CO2 ν3 redshift is estimated. For all values of n, the Ar atoms tend to surround the CO2 molecule. A complete first solvation shell is first found for n=14, and the largest complete first solvation shell is found for n=17. Although the most recent semiempirical CO2–Ar potential function of Hutson et al. [J. Chem. Phys. 105, 9130 (1996)] gives more accurate predictions of spectroscopic properties for n=1 than the best available ab initio potential function [Marshall et al., J. Chem. Phys. 104, 6569 (1996)], both potential functions give quite similar predictions for structures and approximate CO2 ν3 redshifts for larger values of n.

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          Most cited references26

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          A highly accurate interatomic potential for argon

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            Quantum Monte Carlo studies of vibrational states in molecules and clusters

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              Treatment of rigid bodies by diffusion Monte Carlo: Application to the para‐H2⋅⋅⋅H2O and ortho‐H2⋅⋅⋅H2O clusters

              V. Buch (1992)
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                Author and article information

                Journal
                The Journal of Chemical Physics
                AIP Publishing
                0021-9606
                1089-7690
                July 22 1998
                July 22 1998
                July 22 1998
                July 22 1998
                : 109
                : 4
                : 1343-1351
                Article
                10.1063/1.476686
                fe4daa43-975b-48ae-93bd-a871a44629d3
                © 1998
                History

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