Answers are grounded in this paper and cite their sources.
Results of extensive high-resolution synchrotron radiation photoemission studies reveal significant differences between Au/InP(110) interfaces formed at 300 and at 60 K. At 300 K, Au atom deposition results in substantial substrate disruption and, for coverages ≥2 Å, a thickening Au overlayer containing intermixed In and P atoms. For atom deposition at 60 K, the amount of substrate disruption is not significantly changed, but surface segregation of the released In and P atoms is largely, though not entirely, inhibited. These reults show that the distinctly different temperature-dependent Schottky barrier evolution on n- and p-type InP(110) cannot be attributed to thermally controlled reaction since there is little such control. Low-temperature changes in Fermi-level pinning for Au coverages at 2–4 Å appear related to the development of metallic character in the overlayer.
No takes yet. Share an insight, caveat, or question.
Waddill et al. (1989) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: