The authors have evaporated submonolayer to monolayer Sb films on the clean Au(110) surface and investigated the resultant Sb-induced reconstructions using low energy electron diffraction, x-ray photoelectron spectroscopy, Auger electron spectroscopy, and surface x-ray diffraction. They discovered a sequence of reconstructions, namely,
c(2×2),
(
×
)R54.7°,
(
), and
p(5×6), with increasing coverage of Sb. The well-known
(2×1) reconstruction of the clean Au(110) surface changes to
c(2×2) at an Sb coverage of
θ ≈ 0.5 ML. At higher Sb coverages, there is a phase transition from
c(2×2) to
(
×
)R54.7°, with the
(
×
)R54.7° pattern emerging at an Sb coverage of
θ ≈ 0.7 ML. Upon further deposition, the superstructure spots of the
(
×
)R54.7° reconstruction each split into two, resulting in the
(
) pattern at a coverage of
θ ≈ 0.8 ML. Finally, an
Sb/Au(110)-p(5×6) reconstruction emerges at coverages in excess of 1 ML. They have also studied the temperature dependence of the
c(2×2) surface phase.