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Food Lipids: Chemistry, Nutrition, and Biotechnology

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Generally, it is accepted that both homogeneous <strong>and</strong> heterogeneous forms of<br />

nucleation occur. The former occurs in the absence of any foreign particle surfaces.<br />

The latter type occurs in practical systems when nuclei develop on the surface of<br />

solid impurities that are present. Chemical nucleation has also been referred to as a<br />

third, distinct type of nucleation [4]. Unlike heterogeneous nucleation, chemical nucleation<br />

results when organic agents that were added to a system dissolve <strong>and</strong> chemically<br />

react, activating the polymer. The ionic chain ends, which develop from polymer<br />

chain scission, aggregate <strong>and</strong> form nuclei. Therefore, it appears that chemical<br />

nucleation simply refers to chemical induction of heterogeneous nuclei rather than<br />

the more direct physical addition of solid heterogeneous nuclei.<br />

Both primary <strong>and</strong> secondary nucleation have been described by many authors<br />

[1–3]. Secondary nucleation is relatively simple to underst<strong>and</strong>. It results from fracture<br />

of growing crystals into smaller stable crystal nuclei. Nuclei stability is a function<br />

of nuclei solubility. This solubility, in turn, depends on the nuclei size at a given<br />

temperature. Nucleation theory addresses the concept of critical size regarding the<br />

development of stable primary nuclei.<br />

An elegant discussion of these concepts was presented by Timms [2]. Two<br />

opposing actions exist when molecules attempt to aggregate. The first, energy evolution<br />

due to the heat of crystallization, favors crystallization as energy is released<br />

from the aggregating embryo. The second action, that of molecular surface enlargement,<br />

requires energy input to overcome surface tension or pressure. A stable nuclei<br />

will form only when the heat of crystallization is greater than the energy required<br />

to overcome surface energy. This relationship is represented in Eq. (3):<br />

3<br />

2 4�r �Gv �G embryo =4�r � � (3)<br />

3Vm where the first term on the right represents the surface energy contributions <strong>and</strong><br />

the second depicts the volume contributions of the heat of fusion. Defining terms,<br />

�G embryo is the Gibbs free energy of the embryo, r is the radius of the nucleus, � is<br />

the surface free energy per unit surface area, �G v is the molar free energy change<br />

resulting from the melt–solid phase change, <strong>and</strong> V m is the molar volume [3]. The<br />

overall free energy will reach a maximum at some critical embryo size. Free energy<br />

will then tend toward a minimum in all embryos. This occurs through melting of<br />

smaller embryos or continued growth of embryos greater than the critical size.<br />

C. Crystal Growth<br />

Crystal growth continues as the properly configured crystallizing molecule diffuses<br />

to the proper place on the growing crystal surface. The rate of growth is directly<br />

proportional to supercooling <strong>and</strong> varies inversely with viscosity, since molecular<br />

diffusion is reduced as melt viscosity increases. Equation (2) predicts that small<br />

amounts of supercooling will lead to larger crystals versus greater supercooling leading<br />

to smaller crystals. These crystals will be relatively perfect, since the crystal<br />

attachment surface can become more precisely configured with the slower crystallization<br />

rate. Greater supercooling, by contrast, affords faster crystallization (provided<br />

the viscosity remains adequate for molecular diffusion) but also results in more<br />

crystal faults. Faults can arise as molecules from the melt attach to the crystal surface<br />

Copyright 2002 by Marcel Dekker, Inc. All Rights Reserved.

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