Hi Davide,
The ideal gas equation of state (which GRI30 utilizes) assumes that all species activity coefficients are unity, so the chemical potential of a species mu_k is:
mu_k = mu^o_k + RT ln(C_k / C^o_k)
where mu^o_k is the chemical potential at the standard / reference state, which is determined from inputs in the cti file (via NASA polynomials, for GRI30, but other options exist).
C_k is the species molar concentration (or molar density, in Cantera’s parlance), C_k = X_k*P/R/T (where X_k is mole fraction, P is pressure, R the universal gas constant and T the temperature).
C^o_k is the molar concentration of species k at the reference state, which is at the reference pressure P^o, the current temperature, and assumes a mole fraction of 100%. i.e. C^o_k = P^o/R/T.
Putting it all together, the chemical potential is:
mu_k = mu^o_k + RTln(P*X_k/P^o)
IMHO, this should be spelled out in the
science section of Cantera's website, but we just haven’t gotten there, yet.
Thanks - hope this helps,
Steven
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Steven DeCaluwe, PhD | Associate Professor of Mechanical Engineering
COLORADOSCHOOLOFMINES
Brown Building W410B
Golden, CO 80401