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Computer Simulations, Scaling and the Prediction of Nucleation Rates
Barbara Hale Physics Department and Cloud and Aerosol Sciences Laboratory University of Missouri – Rolla Rolla, MO USA
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Nucleation : formation of embryos of the new phase from the metastable (supersaturated) parent phase
K. Yasuoka and M. Matsumoto, J. Chem. Phys. 109, 8451 (1998)
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“Molecular dynamics of homogeneous nucleation in the vapor phase: Lennard-Jones fluid”, K. Yasuoka and M. Matsumoto, J. Chem. Phys. 109, 8451 (1998);
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Estimating the nucleation rate, J, from the molecular dynamics simulation at T = 80.3K. Supersaturation ratio = P/Po = 6.8 vol. = ( 60 x 60 x 60) 3;
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Nucleation is a non-equilibrium process!
●There is no “first principles” theory from which to determine the nucleation rate. ● Most models attempt to treat nucleation as the decay of a near-equilibrium metastable (supersaturated) state. ● The classical nucleation theory (CNT) model was first developed in by Volmer and Weber, and by Becker and Döring in …. following a proposal by Gibbs. ● CNT treats nucleation as a fluctuation phenomenon in which small embryos of the new phase overcome free energy barriers and grow irreversibly to macroscopic size.
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Classical Nucleation Theory
(vapor-to-liquid) Jclassical = [N1 v 4rn*2/3 ] · Nn* = [Monomer flux] · [# Critical Clusters/Vol.]
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Estimating Nn Nn / N1 = exp [–Work of formation / kT]
Work of formation of cluster from vapor: W(n) = 4 rn2 n kT ln S S = P/Po
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n* = critical sized cluster has equal probability of growing or decaying
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n* = critical sized cluster
at n = n*: dW(n) / dn = 0 Let W(n) = An2/3 -nlnS where A = [36]1/3 liq-2/3 /kT liq= liquid number density
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Volume / Surface in W(n*)
d/dn [ An2/3 - nlnS]n* = 0 (2/3)A n*-1/3 = lnS n* = [2A/ 3lnS]3 W(n*) /kT = ½ n* lnS = [16/3] [/(liq2/3 kT) ]3 / [lnS]2 liq= liquid number density
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Classical Nucleation Rate
(T) a – bT is the bulk liquid surface tension ;
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Homogeneous Nucleation rate data for water: classical nucleation rate model has wrong T dependence
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Motivation for Scaling J at T << Tc
The CNT nucleation rate depends exponentially on (T)3 / [ln (P/Po(T))]2 . To obtain a physically realistic T dependence of J, a good starting point is to require functional forms for (T) and Po(T) which reflect “universal” properties of surface tension and vapor pressure.
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Scaling of the surface tension at T << Tc
Assume a scaled form for : = o’ [Tc- T] with =1 for simplicity. Many substances fit this form and the critical exponent (corresponding to ) is close to 1. = excess surface entropy per molecule / k 2 for normal liquids for substances with dipole moment (a law of corresponding states result; Eötvös 1869)
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Scaled Nucleation Rate at T << Tc B. N. Hale, Phys
Scaled Nucleation Rate at T << Tc B. N. Hale, Phys. Rev A 33, 4156 (1986); J. Chem. Phys. 122, (2005) J0,scaled [thermal (Tc)] -3 s-1 “scaled supersaturation” lnS/[Tc/T-1]3/2
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Water nucleation rate data of Wölk and Strey plotted vs
Water nucleation rate data of Wölk and Strey plotted vs. lnS / [Tc/T-1]3/2 ; Co = [Tc/240-1]3/2 ; Tc = K J. Chem. Phys. 122, (2005)
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Toluene (C7H8) nucleation data of Schmitt et al plotted vs
Toluene (C7H8) nucleation data of Schmitt et al plotted vs. scaled supersaturation, Co = [Tc /240-1]3/2 ; Tc = 591.8K
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Nonane (C9H20) nucleation data of Adams et al. plotted vs
Nonane (C9H20) nucleation data of Adams et al. plotted vs. scaled supersaturation ; Co = [Tc/240-1]3/2 ; Tc = 594.6K
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for most materials (corresponding states)
Comparison of Jscaled with water data from different experimental techniques: plot log[J/J0,scaled] vs. J0,scaled cm-3 s-1 for most materials (corresponding states)
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Missing terms in the classical work of formation?
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Monte Carlo Simulations
Ensemble B: n cluster with probe interactions normal Ensemble A: (n -1) cluster plus monomer probe interactions turned off Calculate f(n) =[F(n)-F(n-1)]/kT
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Monte Carlo Helmholtz free energy differences for small water clusters: f(n) =[F(n)-F(n-1)]/kT B.N. Hale and D. J. DiMattio, J. Phys. Chem. B 108, (2004)
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Nucleation rate via Monte Carlo
Calculation of Nucleation rate from Monte Carlo -f(n) : Jn = flux · Nn* Monte Carlo = [N1v1 4rn2 ] · N1 exp 2,n(-f(n´) – ln[liq/1o]+lnS) J = [n Jn ]-1 The steady-state nucleation rate summation procedure requires no determination of n* as long as one sums over a sufficiently large number of n values.
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Monte Carlo TIP4P nucleation rate results for experimental water data points (Si,Ti)
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Comments & Conclusions
Experimental data indicate that Jexp is a function of lnS/[Tc/T-1]3/2 A “first principles” derivation of this scaling effect is not known; Monte Carlo simulations of f(n) for TIP4P water clusters show evidence of scaling; Temperature dependence in pre-factor of classical model can be partially cancelled when energy of formation is calculated from a discrete sum of f(n) over small cluster sizes. Can this be cast into more general formalism?
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Molecular Dynamics Simulations
Solve Newton’s equations, mi d2ri/dt2 = Fi = -i j≠i U(rj-ri), iteratively for all i=1,2… n atoms; Quench the system to temperature, T, and monitor cluster formation. Measure J rate at which clusters form
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