The effects of pressure on phase stability of an HgSn alloy with nearly equiatomic
composition have been studied up to 30 GPa with diamond anvil cells using x-ray powder
diffraction with synchrotron radiation. A Hg-rich phase hR 1-(Hg) with a rhombohedral
distortion of a face-centred cubic (fcc) cell is found to form in the alloy at pressures above
3 GPa in coexistence with a Sn-rich phase with a simple hexagonal structure sh-hP 1
stable at ambient pressure. While the sh-hP 1 phase transforms at pressures above
15 GPa to a body-centred tetragonal bct-tI 2 phase, the hR 1-(Hg) phase remains
stable up to 30 GPa. The hR 1-(Hg) phase is regarded as a solid solution of Sn in
α-Hg.
The range of solubility is estimated from about 5 to 10 at.% Sn. The alloying of Hg with Sn stabilises the
α-Hg
phase up to pressure of 30 GPa, while pure
α-Hg
becomes unstable at 3.7 GPa transforming to a bct (tI 2) phase. The
hR 1-(Hg) phase reveals a strong anisotropy on compression. An increase of
c/a from
1.99 to 2.25 in the pressure range from 2.6 to 29.9 GPa is observed displaying a trend towards fcc with
c/a = 2.45
in a primitive rhombohedral setting (hexagonal axes).
The stabilisation of the hR 1-(Hg) phase by alloying with Sn and the range of solubility of Sn in
α-Hg
are discussed within the concept of Fermi sphere–Brillouin zone interactions.