Abstract
The structure of the liquid Hg/sapphire interface was measured with angstrom-scale resolution by high-energy X-ray reflectivity. The atomic Hg layering found at the interface is less pronounced than at the Hg/vapor interface, showing a twice-shorter decay length with depth, and a weaker peak/valley density contrast. We also find a near-interface, 8 ± 3 Å thick layer, the density of which, although depth-varying, is enhanced, on average, by 10 ± 5% relative to the bulk. The enhancement is assigned to a 0.13 ± 0.05 e/atom charge transfer from the Hg to the substrate, somewhat less than theory. The unexplained anomalous temperature dependence previously reported for the mercury/vapor density profile is absent here, implying a nonstructural origin for the anomaly.
| Original language | English |
|---|---|
| Pages (from-to) | 1041-1045 |
| Number of pages | 5 |
| Journal | Journal of Physical Chemistry Letters |
| Volume | 1 |
| Issue number | 7 |
| DOIs | |
| State | Published - 1 Apr 2010 |
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