Thanks for the explanation, Jonathan. I think I see what you mean. I'm 
now trying to extend the quaternary example to the dynamic case, as in 
the binary example, such that the interface can move after 
equilibration. However, in this case there is no definition of melting 
temperature, and simply lowering the starting temperature does not cause 
the interface to move. Some experimentation with temperature values 
suggests that higher temperature creates a sharper, narrower interface 
while lower temperature creates a broader interface, but it always 
remains centered.

I imagine this must be related to the different enthalpy terms between 
the binary and quaternary cases? In the binary case the average enthalpy 
is 0 for equilibration and < 0 in order to grow the solid phase 
(interface moves right). Raising the temperature above Tm gives enthalpy 
 > 0 and shrinks the solid phase (interface moves left). This makes 
sense as it is defined as proportional to the undercooling which is 
giving the driving force for phase change.

In contrast, the average enthalpy as defined in the quaternary case 
seems to be > 0 for any positive temperature, yet the interface doesn't 
move. So I suppose my next question is, why does the role of enthalpy 
appear to change between the binary and quaternary cases, and how to go 
about modifying the quaternary approach to account for melting temp, 
undercooling, driving force, moving interface, etc?

Thanks for being so responsive and patient with a phase-field newcomer.

Adam


On 11/15/2012 09:00 AM, Jonathan Guyer wrote:
> On Nov 14, 2012, at 6:25 PM, Adam Stone wrote:
>
>> I'm going through the quaternary phase field example and having some 
>> difficulty understanding the calculation of standard potentials.
> :
> :
>> But I don't understand how you "cook" these standard potentials:
>>
>> for Cj in interstitials + substitutionals + [solvent]:
>> ...     Cj.standardPotential = R * T * (numerix.log(Cj.L/rhoL)
>> ...                                     - numerix.log(Cj.S/rhoS))
>>
>> Since this is the difference between the solid and liquid potentials, any 
>> terms common to both would have disappeared and we should be left with the 
>> remaining terms unique to each phase. But if these are indeed "standard" 
>> potentials for the solid and liquid, it seems like none of them should 
>> include R*T*ln(C/p) terms in the first place? So I don't see how this 
>> expression is obtained (or why the solid term is being subtracted from the 
>> liquid term rather than vice versa).
> This is just a statement of equality of chemical potentials in equilibrium. 
> The difference between the standard potentials must be equal to the log of 
> the ratio of the concentrations in equilibrium (for the ideal solution 
> considered in that example, anyway). We start this example with the ansatz 
> that an 0.3-0.4-0.2-0.1 solid is in equilibrium with a 0.4-0.3-0.1-0.2 liquid.
>
> The standard states of different phases are not in equilibrium; if they were, 
> then vapor pressure would be a useless concept (pure bcc iron would be in 
> equilibrium with 1 atm of Fe vapor under the same conditions that pure liquid 
> helium was in equilibrium with 1 atm of He gas). We pick standard states 
> because we need something to compare to, but they can't all have the same 
> values or there would be no chemical specificity.
>
> It is also not true that the R*T*ln(C/p) terms don't appear in the standard 
> state. It's just that, as a matter of convention, we usually take the 
> standard state of condensed phases to have a unit activity and of gaseous 
> phases to be at 1 atm and so the logs are zero. That's only because we chose 
> to compare pressures in units of atmospheres, though; you don't have to.
>
>
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