1994/12/31 by B. Diekmann, P. Borrmann, Diekmann, B. +5
Chemistry · Earth and Planetary Sciences · Physics and Astronomy · #Advanced Chemical Physics Studies #Atmospheric Ozone and Climate #Condensed Matter (cond-mat) #FOS: Physical sciences #Molecular Spectroscopy and Structure #cond-mat
paper · pdf · doi:10.48550/arxiv.cond-mat/9412123
9 pages, LaTeX, uses REVTEX, coloured postscript figures (also printable in bw) available at http://www.physik.uni-oldenburg.de/Docs/documents/UOL-THEO3-94-5/Figures.uu, article (html-form) available at http://www.physik.uni-oldenburg.de/Docs/documents/UOL-THEO3-94-5/cont.html
arxiv created 1994/12/31 · openalex publication_date 1994/12/31 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Geometries and energies for H3+(H2)n clusters (n = 0, ..., 11) have been calculated using standard "ab initio" methods. Up to clusters with n = 6, four different Pople basis sets (DZ, TZ, TZP) have been used in the calculations. For larger cluster sizes, the calculations have been carried out with one basis set (DZ) using the HF/CISD method. We discuss here only the nice counterplay of polarisation effects between the central H3+ ion and the adsorbed H2 molecules, which naturally governs both the geometric structure and the energy of the clusters.