Carbonatitic
and carbonated silicate melts generated from melting
in the mantle are the chief agents for liberating carbon from the
solid Earth and exert important controls on Earth’s deep carbon
cycle. However, significant gaps in our knowledge about the carbonatitic
melts under conditions pertinent to Earth’s deep interior remain
due to experimental challenges. Here, we report on a first-principles
molecular dynamics (FPMD) calculation of calcium carbonate (CaCO3) melts at pressures up to 52.5 GPa. Our FPMD calculations
reproduce the ultralow viscosity measured by experiments and confirm
the ideal liquid behavior of calcium carbonate melts at pressures
below 11.2 GPa. However, calcium carbonate melts are characterized
by a pronounced nonideal liquid behavior at pressures above 11.2 GPa,
arising from (1) the temporal formation of small carbonate clusters
and (2) increased interactions between Ca2+ and CO3
2– ions. It is found that the Stokes–Einstein
equation relating the viscosity with the diffusion coefficients still
holds at high pressure provided that a suitable effective particle
size can be chosen.