This work is concerned with four molten monohalides with different ionic ra
dii ratios (RbCl, NaI, AgCl, and CuCl) and ideal isotopic systems of these
salts with different ionic mass ratios. The velocity autocorrelation functi
ons of the two ionic species in each melt have been studied by both a theor
etical approximation and molecular dynamics simulations. It is found that t
heir main features may be qualitatively predicted by considering suitable c
ombinations of the second and fourth frequency moments of their spectra. Th
e analysis of these two parameters allows us to determine how the structure
(strongly dependent on the ionic size difference) and the ionic masses con
tribute to the shape of the velocity autocorrelation functions. The results
show that the averaged microscopic motion of the small ions is mainly dete
rmined by the first neighboring shell of unlike ions, whereas the nearest s
hell of like ions also affects the dynamics of the large ions. This effect
is more pronounced as the size difference is greater. Furthermore, it is co
ncluded that the size differences encourage the rattling motion of the larg
e ions, whereas the mass difference encourages the backscattering and oscil
lations of the velocity autocorrelation function of the light ions. A simpl
e rule is derived to determine the interplay between these two effects. Com
parison between the mass and nearest distance ratios enables the prediction
as to which species will experience a more pronounced backscattering motio
n. The size difference effects prevail in the hydrodynamics regime and the
self-diffusion coefficient of the small ions is higher than that of the lar
ge ones. The difference between the self-diffusion coefficient increases as
the size differences increases. (C) 2000 American Institute of Physics. [S
0021-9606(00)50347-X].