Abstract

Recently, for calculating the effective pair interactions in liquid transition metals, we have developed an approach which includes the Wills-Harrison and Bretonnet-Silbert models as limit cases. Here, we apply this approach to noble liquid metals. The dependencies of pair potentials and corresponding MD-simulated pair correlation functions in pure liquid Cu, Ag and Au on the portion of the non-diagonal (with respect to the magnet quantum number) d-d-electron couplings in the metal under consideration are studied. The model provides a good agreement with experimental and ab initio data for pair correlation functions, structure factors and velocity autocorrelation functions.

Highlights

  • At present, theoretical investigations of liquid transition metals and their alloys are being carried out intensively [1,2,3,4,5,6,7,8,9,10,11,12]

  • We used the LiquidLib code [46] to calculate velocity autocorrelation function (VAF, normalized on its initial value) for each metal using both the developed pair potentials and EAMs [43,44,45] and compared the results with those obtained by ab initio molecular dynamics (AIMD) [42]

  • We utilize the modified Wills-Harrison model, which takes into account the non-diagonal d-d-electron couplings between neighboring atoms, to generate effective pair interactions in noble metals, namely Cu, Ag, and Au

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Summary

Introduction

Theoretical investigations of liquid transition metals and their alloys are being carried out intensively [1,2,3,4,5,6,7,8,9,10,11,12]. In works [21,25], only the diagonal matrix elements with respect to the magnet quantum number, m, between d states of neighboring atoms are taken into account. It is correct in the case of the rotational symmetry with axis along the interatomic distance. In [35], it was observed that in the case when all possible non-diagonal couplings are taken into account, the d-electron contribution to the WH effective pair potential vanishes and latter becomes equal to the NFE (i.e., in our case, to the BS) contribution only.

Modification of the Wills-Harrison Model
Conclusions
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