Primary (syn-growth) fluid inclusions in synthetic diamonds, produced
within the field of their thermodynamic stability in a high-pressure s
plit-sphere apparatus using the temperature gradient method, have been
studied by optical microscopy and Raman spectroscopy. Inclusions in t
abular diamond crystals contain CH4 + other higher molecular hydrocarb
ons, whereas inclusions in octahedral and dodecahedral diamonds contai
n only CH4. All inclusions in octahedral and dodecahedral diamonds con
tain graphite, which covers the walls of vacuoles as an opaque film. T
he formation of this film is most likely associated with precipitation
of carbon from fluid on cooling. The obtained results emphasize the p
ossible role of hydrocarbons in the process of diamond crystallization
.