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Focus Papers

Crystal growth nucleation and Fermi energy equalization of intrinsic spherical nuclei in glass-forming melts

Article: 014607 | Received 30 Jun 2008, Accepted 31 Oct 2008, Published online: 22 May 2009
 

Abstract

The energy saving resulting from the equalization of Fermi energies of a crystal and its melt is added to the Gibbs free-energy change ΔG2ls associated with a crystal formation in glass-forming melts. This negative contribution being a fraction ε ls(T) of the fusion heat is created by the electrostatic potential energy −U0 resulting from the electron transfer from the crystal to the melt and is maximum at the melting temperature Tm in agreement with a thermodynamics constraint. The homogeneous nucleation critical temperature T2, the nucleation critical barrier ΔG2ls∗/kBT and the critical radius R2ls are determined as functions of εls(T). In bulk metallic glass forming melts, εls(T) and T2 only depend on the free-volume disappearance temperature T0l, and εls(Tm) is larger than 1 (T0l>Tm/3); in conventional undercooled melts εls(Tm) is smaller than 1 (T0l>Tm/3). Unmelted intrinsic crystals act as growth nuclei reducing ΔG2ls∗/kBT and the nucleation time. The temperature-time transformation diagrams of Mg65Y10Cu25, Zr41.2Ti13.8Cu12.5Ni10Be22.5, Pd43Cu27 Ni10P20, Fe83B17 and Ni melts are predicted using classic nucleation models including time lags in transient nucleation, by varying the intrinsic nucleus contribution to the reduction of ΔG2ls∗/kBT. The energy-saving coefficient ε nm(T) of an unmelted crystal of radius Rnm is reduced when RnmR2ls; εnm is quantified and corresponds to the first energy level of one s-electron moving in vacuum in the same spherical attractive potential −U0 despite the fact that the charge screening is built by many-body effects.

Acknowledgments

Thanks are due to Eric Beaugnon, Philippe Odier, Jean-Louis Soubeyroux, to the referees for manuscript review, and to Jacques Friedel for discussions. Commenting on this paper, Yoshihiko Hirotsu considers that intrinsic nuclei could be identified to ‘medium range order’ (MRO) clusters only if the interface cluster-matrix is very diffuse at room temperature. The MRO cluster size depends on the overheating rate and then, these entities exist above the melting temperature even if the cooling rate tends to slightly modify their radii [Citation49]. The Fe85–B15 kinematic viscosity is irreversible between θ = 0 and θ≅0.23 after an overheating up to θ=0.27 in good agreement with our prediction θ≅εls0=0.3 [Citation50] corresponding to the melting temperature of all surviving crystals.

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