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Astron. Astrophys. 337, 847-858 (1998) Dust formation in stellar windsVII. Kinetic nucleation theory for chemical non-equilibrium in the gas phase
A.B.C. Patzer 1,
A. Gauger 2 and
E. Sedlmayr 1
Received 3 March 1998 / Accepted 19 March 1998 Abstract We present a new theoretical formulation of the nucleation process of solid particles from the gas phase with special emphasis on the effects of chemical non-equilibrium in the gas phase and thermal non-equilibrium between the gas and the clusters or dust grains. In the derivation of the nucleation rates from kinetic theory and from thermodynamic arguments thermal and chemical non-equilibrium are straightforwardly included. A hierarchy of expressions for the stationary nucleation rate is given, ranging from a system of equations, which determines the rate, to an approximate analytic expression in the case of a single dominating growth species, which requires only the time scales of the growth processes and the Gibb's free energy change for the formation of clusters. Key words: molecular
processes Send offprint requests to: A.B.C. Patzer This article contains no SIMBAD objects. Contents
© European Southern Observatory (ESO) 1998 Online publication: August 27, 1998 ![]() |