Calculated electronic structure of Au13 clusters

Ramiro Arratia-Perez, Agustin F. Ramos, and G. L. Malli
Phys. Rev. B 39, 3005 – Published 15 February 1989
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Abstract

The electronic structure of cubo-octahedral and icosahedral Au13 clusters has been investigated by the self-consistent-field molecular-orbital Dirac scattered-wave method. Double-point-groupsymmetry considerations indicate that the icosahedral cluster will undergo static Jahn-Teller distortion, while the cubo-octahedral cluster cannot distort because of a Kramers degeneracy in the ground state. Molecular Zeeman and hyperfine interactions are calculated for the cubo-octahedral Au13 cluster through a first-order perturbation to the Dirac Hamiltonian. The predicted g tensors and Au197 hyperfine tensors are consistent with a nearly isotropic paramagnetic-resonance spectrum. The calculated density-of-states (DOS) curves for the Au13 clusters show similar features to those obtained in photoemission experiments of small clusters of gold. Relativistic effects increase the d-band width by more than 1 eV, and spin-orbit interaction splits the occupied d band by about 2 eV in both clusters. These calculated values are approximately 75% of the observed values for gold in the bulk metal. It is clearly shown that the overlap of the d band by the s-p band is mainly due to relativistic effects.

  • Received 16 August 1988

DOI:https://doi.org/10.1103/PhysRevB.39.3005

©1989 American Physical Society

Authors & Affiliations

Ramiro Arratia-Perez, Agustin F. Ramos, and G. L. Malli

  • Department of Chemistry and Theoretical Sciences Institute, Simon Fraser University, Burnaby, British Columbia, Canada V5A1S6

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Vol. 39, Iss. 5 — 15 February 1989

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