2003
DOI: 10.1016/s0009-2614(03)00692-4
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Quasirelativistic multipartitioning perturbation theory calculations on electronic transitions in Au2

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Cited by 18 publications
(14 citation statements)
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“…However, neither results are in good agreement with the gas phase or matrix absorption spectra, in particular the two intense A and B transitions are not reproduced. It is worth to notice that more elaborate calculations [56][57][58] which take explicitly into account the spin-orbit coupling are in much better agreement with the dimer gas phase experimental absorption spectra. This is a clear indication that the lack of spin-orbit splitting in the TD-DFT calculations results in a serious limitation to reproduce the experimental spectra.…”
mentioning
confidence: 64%
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“…However, neither results are in good agreement with the gas phase or matrix absorption spectra, in particular the two intense A and B transitions are not reproduced. It is worth to notice that more elaborate calculations [56][57][58] which take explicitly into account the spin-orbit coupling are in much better agreement with the dimer gas phase experimental absorption spectra. This is a clear indication that the lack of spin-orbit splitting in the TD-DFT calculations results in a serious limitation to reproduce the experimental spectra.…”
mentioning
confidence: 64%
“…The gold dimer has been calculated, including the excited states, using Hartree-Fock and DFT methods. [56][57][58][59] Similar techniques were applied to determine the ground state geometries of the trimer, 60-63 the tetramer, 60,62,64 and the pentamer. 62,64 DFT calculations have been performed more recently in order to predict the lowest energy structures 12-14, 16, 18, 19, 31 and to calculate the optical spectra by TFD-DFT for clusters up to Au 14 and Au 20 .…”
Section: Comparison To Td-dft Calculationsmentioning
confidence: 99%
“…A state-selective effective Hamiltonian is built in a model space spanned by Slater determinants following the procedure reported in Ref. [12]. The spin-orbit interactions between the model and outer spaces are completely neglected.…”
Section: Computational Detailsmentioning
confidence: 99%
“…The spin-orbit interactions between the model and outer spaces are completely neglected. Therefore, additional requirements on the model space and a procedure for its composition are imposed [12]. The procedure employed is based on the spin-orbit-free iterative perturbative configuration selection against a threshold [13].…”
Section: Computational Detailsmentioning
confidence: 99%
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