Hi,
Could you please attach the input data file, CaCO3-calcination-surface.yaml?
Thanks,
Ray
Thanks Ray, it makes sense.
The pressure dependence of the pressure on Gibbs energy can be seen from the fundamental equation.
dG = Vmdp - SdT
for an ideal gas Vm = RT/p giving a pressure dependence of ΔG = RT·ln(p/po)
for an incompressible solid ΔG = Vm(p - po)
Below is shown the standard_gibbs_RT from Cantera as function of pressure showing these relationships.
The reason for the question was that the overall reaction CaCO3 <=> CO2 + CaO, shifted to the right ( or at least I got a net_production of CO2) at very high pressures contrary to common knowledge. I think the reason for Cantera getting this wrong result is the lack of pressure dependence on the surface species. The surface species have no molar volume associated with them and therefore a simple model will leave the Gibbs energy independent of the pressure as is also noted on the graph. But that fine and I can live with it. Now I understand how Cantera works and know that you should be cautious at high pressures.
Tom, yes, you should be cautious calculating K from exp(-ΔG/RT), but in this case it is ok because the activity of CaO is fixed and there is one surface specie on both side of the reaction.
Best regards
Mikael