Recent studies of microdiamonds from orogenic belts related to continental collisions induced experimentalists to explore new crystallization media possible for diamond synthesis. This has led to considerable progress in diamond-synthesis experiments under high pressures and high temperatures. Diamond was found to grow in a wide variety of systems, which drastically differ from the metal-solvent-catalyst media that have been known since the 1950s in industrial diamond syntheses. The newer systems include a variety of melts consisting of silicate, carbonate, sulfur-carbon, as well as carbon-oxygen-hydrogen (C-O-H) supercritical fluid systems in the presence of different oxides. Our experimental program has focused on systems compositionally approximating natural sites of ultrahigh-pressure metamorphic rocks, where abundant microdiamonds occur. Yet to be explored are SiO2-rich systems that constitute an important diamond-bearing lithology in the world-famous Kokchetav ultrahigh-pressure metamorphic (UHPM) terrane. The purpose of this study is to determine what effect the presence of SiO2 has on the synthesis of diamond from C-O-H supercritical fluid. Experiments performed in a Walker-style multianvil apparatus at T = 1450-1500°C and P = 8-8.5 GPa on the Si-C-O-H system at different levels of oxygen fugacity (fO2) have led us to the conclusion that diamond crystallization requires more reduced media than its counterpart synthesized in Mg-C-O-H and Ca-Mg-C-O-H systems at similar pressures, temperatures, and times.
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Dobrzhinetskaya et al. (2007) studied this question.
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