Formation and Evolution of Minerals in Accretion Disks and Stellar Outflows

The contribution discusses dust formation and dust processing in oxygen rich stellar outflows under non-explosive conditions, and in circumstellar discs. The main topics are calculation of solid-gas chemical equilibria, the basic concepts for calculating dust growth under non-equilibrium conditions, dust processing by annealing and solid diffusion, a discussion of non-equilibrium dust formation in stellar winds, and in particular a discussion of the composition and evolution of the mineral mixture in protoplanetary accretion discs. An overview is given over the data on dust growth, annealing, and on solid diffusion for astrophysically relevant materials available so far from laboratory experiments.

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