The structure and dynamics of superionic α-CuI were studied in detail by means of
ab initio Born–Oppenheimer molecular dynamics simulations. The extreme cation
disorder and a soft immobile face centred cubic sub-lattice were evident from the
highly diffuse atomic density profiles. The Cu–Cu pair distribution function and
distribution of Cu–I–Cu bond angles possess distinct peaks at 2.6Å and 60°
respectively, which were markedly lower than the values expected from the
average cationic density, pointing to the presence of pronounced short-range
copper–copper correlations. Comparison with lattice static calculations showed that
these correlations and the marked shift in the cationic density profile in the <111>
directions were associated with a locally distorted cation sub-lattice, and that the
movements within the tetrahedral cavities involve rapid jumps into and out of
shallow basins on the system potential energy surface. On average, the iodine
atoms were surrounded by three copper atoms within their first coordination shell,
with the fourth copper atom being located in a transition zone between two
neighbouring iodine cavities. However, time-resolved analysis revealed that the
local structure actually involves a mixture of threefold-, fourfold-and fivefoldcoordinated
iodine. Examination of the ionic trajectories showed that the copper
ions jump rapidly to nearest neighbouring tetrahedral cavities (aligned in the <100>
directions) following a markedly curved trajectory and often involving short-lived
(~1ps) interstitial positions. The nature of the correlated diffusion underlying the
unusually high fraction of coppers with short residence time can be attributed to the
presence of a large number of 'unsuccessful' jumps and the likelihood of
cooperative motion of pairs of coppers. The calculated diffusion coefficient at
750K, DCu = 2.8 x 10−5cm2/s, was in excellent agreement with that found
experimentally.
Diffusion within α-CuI Studied Using Ab Initio Molecular Dynamics Simulations.
C.E.Mohn, S.Stølen, S.Hull: Journal of Physics - Condensed Matter, 2009, 21[33],
335403