4.7 Article

Two- and three-body interatomic dispersion energy contributions to binding in molecules and solids

Journal

JOURNAL OF CHEMICAL PHYSICS
Volume 132, Issue 23, Pages -

Publisher

AIP Publishing
DOI: 10.1063/1.3432765

Keywords

binding energy; crystal structure; DNA; graphene; helium neutral molecules; intermolecular forces; intramolecular forces; neon; potential energy functions; proteins; van der Waals forces

Funding

  1. SNL [120209]
  2. United States Department of Energy [DE-AC04-94AL85000]
  3. Alexander von Humboldt (AvH) foundation

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We present numerical estimates of the leading two- and three-body dispersion energy terms in van der Waals interactions for a broad variety of molecules and solids. The calculations are based on London and Axilrod-Teller-Muto expressions where the required interatomic dispersion energy coefficients, C-6 and C-9, are computed on the fly from the electron density. Inter- and intramolecular energy contributions are obtained using the Tang-Toennies (TT) damping function for short interatomic distances. The TT range parameters are equally extracted on the fly from the electron density using their linear relationship to van der Waals radii. This relationship is empiricially determined for all the combinations of He-Xe rare gas dimers, as well as for the He and Ar trimers. The investigated systems include the S22 database of noncovalent interactions, Ar, benzene and ice crystals, bilayer graphene, C-60 dimer, a peptide (Ala(10)), an intercalated drug-DNA model [ellipticine-d(CG)(2)], 42 DNA base pairs, a protein (DHFR, 2616 atoms), double stranded DNA (1905 atoms), and 12 molecular crystal polymorphs from crystal structure prediction blind test studies. The two- and three-body interatomic dispersion energies are found to contribute significantly to binding and cohesive energies, for bilayer graphene the latter reaches 50% of experimentally derived binding energy. These results suggest that interatomic three-body dispersion potentials should be accounted for in atomistic simulations when modeling bulky molecules or condensed phase systems. (C) 2010 American Institute of Physics. [doi: 10.1063/1.3432765]

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