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Influence of the Processes Parameters on the Properties of The ...

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Chapter 2.<br />

<str<strong>on</strong>g>Processes</str<strong>on</strong>g> to Manufacture Foams and to Functi<strong>on</strong>alize <str<strong>on</strong>g>the</str<strong>on</strong>g> Surface<br />

4.3 Nucleati<strong>on</strong><br />

As we have explained earlier, when <str<strong>on</strong>g>the</str<strong>on</strong>g> pressure is reduced from <str<strong>on</strong>g>the</str<strong>on</strong>g> equilibrium state, <str<strong>on</strong>g>the</str<strong>on</strong>g><br />

formati<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> nuclei occurs as a result <str<strong>on</strong>g>of</str<strong>on</strong>g> supersaturati<strong>on</strong>. This number <str<strong>on</strong>g>of</str<strong>on</strong>g> nuclei can be calculated by using<br />

<str<strong>on</strong>g>the</str<strong>on</strong>g> classical nucleati<strong>on</strong> <str<strong>on</strong>g>the</str<strong>on</strong>g>ory <str<strong>on</strong>g>of</str<strong>on</strong>g> <str<strong>on</strong>g>the</str<strong>on</strong>g> physical chemistry. <strong>The</strong> number <str<strong>on</strong>g>of</str<strong>on</strong>g> pores generated can be modeled by<br />

calculating <str<strong>on</strong>g>the</str<strong>on</strong>g> number <str<strong>on</strong>g>of</str<strong>on</strong>g> nuclei generated.<br />

In <str<strong>on</strong>g>the</str<strong>on</strong>g> classical nucleati<strong>on</strong> <str<strong>on</strong>g>the</str<strong>on</strong>g>ory, <str<strong>on</strong>g>the</str<strong>on</strong>g> free energy <str<strong>on</strong>g>of</str<strong>on</strong>g> <str<strong>on</strong>g>the</str<strong>on</strong>g> formati<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> a cluster <str<strong>on</strong>g>of</str<strong>on</strong>g> radius r in a<br />

closed iso<str<strong>on</strong>g>the</str<strong>on</strong>g>rmal system in chemical equilibrium is given by Tsivintzelis et al. [2007a] and Adams<strong>on</strong> and<br />

Gast [1997]:<br />

3<br />

4 r<br />

G P<br />

4r<br />

2 <br />

(2.17)<br />

3<br />

where r is <str<strong>on</strong>g>the</str<strong>on</strong>g> radius <str<strong>on</strong>g>of</str<strong>on</strong>g> <str<strong>on</strong>g>the</str<strong>on</strong>g> spherical cluster, γ is <str<strong>on</strong>g>the</str<strong>on</strong>g> interfacial tensi<strong>on</strong> and ΔP is <str<strong>on</strong>g>the</str<strong>on</strong>g> pressure between <str<strong>on</strong>g>the</str<strong>on</strong>g><br />

two sides <str<strong>on</strong>g>of</str<strong>on</strong>g> <str<strong>on</strong>g>the</str<strong>on</strong>g> interface.<br />

radius r c :<br />

When ΔG is plotted against cluster size, <strong>on</strong>e obtains a curve that shows a maximum at a critical<br />

dG<br />

dr<br />

2<br />

0 rc<br />

<br />

(2.18)<br />

P<br />

Equati<strong>on</strong> 2.18 is <str<strong>on</strong>g>the</str<strong>on</strong>g> Young-Laplace equati<strong>on</strong>. <strong>The</strong> maximum value <str<strong>on</strong>g>of</str<strong>on</strong>g> ΔG for homogenous<br />

nucleati<strong>on</strong> is obtained by substituting equati<strong>on</strong> 2.17 into equati<strong>on</strong> 2.19):<br />

G<br />

*<br />

hom<br />

3<br />

16<br />

<br />

2<br />

3P<br />

(2.19)<br />

<strong>The</strong> interfacial tensi<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> <str<strong>on</strong>g>the</str<strong>on</strong>g> mixture is calculated by <str<strong>on</strong>g>the</str<strong>on</strong>g> following equati<strong>on</strong> given by Goel and<br />

Beckman [1994a]:<br />

<br />

<br />

<br />

<br />

<br />

<br />

<br />

4<br />

mix<br />

4<br />

<br />

mix<br />

<br />

polymer<br />

( 1 wCO2<br />

)<br />

(2.20)<br />

<br />

polymer<br />

where ρ are <str<strong>on</strong>g>the</str<strong>on</strong>g> densities and w CO2s is <str<strong>on</strong>g>the</str<strong>on</strong>g> weight fracti<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> CO 2 absorbed by <str<strong>on</strong>g>the</str<strong>on</strong>g> polymer.<br />

<strong>The</strong> surface tensi<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> PLGA 50:50 can be taken as 35.3 N/m as reported by Vargha-Butler et al.<br />

[2001]. <strong>The</strong> interfacial tensi<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> CO 2 is essentially zero at supercritical state, thus it will not be introduced<br />

in <str<strong>on</strong>g>the</str<strong>on</strong>g> equati<strong>on</strong>. A more complicated model which predicts <str<strong>on</strong>g>the</str<strong>on</strong>g> depressi<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> interfacial tensi<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> a polymer<br />

as a functi<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> CO 2 sorpti<strong>on</strong> is proposed by Harris<strong>on</strong> et al. [1996]. Unfortunately, this model requires<br />

experimental data for <str<strong>on</strong>g>the</str<strong>on</strong>g> depressi<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> <str<strong>on</strong>g>the</str<strong>on</strong>g> interfacial tensi<strong>on</strong> as a functi<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> CO 2 and will not be<br />

c<strong>on</strong>sidered here.<br />

1994a]:<br />

Steady state rate <str<strong>on</strong>g>of</str<strong>on</strong>g> nucleati<strong>on</strong> can be described by <str<strong>on</strong>g>the</str<strong>on</strong>g> following equati<strong>on</strong> [Goel and Beckman,<br />

*<br />

G<br />

<br />

hom<br />

N <br />

0<br />

Cf<br />

0<br />

exp (2.21)<br />

kT <br />

- 53 -

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