cantera/src/equil/vcs_TP.cpp
2012-12-15 00:49:14 +00:00

186 lines
6.5 KiB
C++

#include "cantera/equil/vcs_solve.h"
#include "cantera/equil/vcs_internal.h"
#include "cantera/equil/vcs_species_thermo.h"
#include "cantera/equil/vcs_VolPhase.h"
#include <cstdio>
#include <cstdlib>
#include <cmath>
namespace VCSnonideal
{
/*****************************************************************************/
/*****************************************************************************/
/*****************************************************************************/
int VCS_SOLVE::vcs_TP(int ipr, int ip1, int maxit, double T_arg, double pres_arg)
/**************************************************************************
*
* vcs_TP:
*
* Solve an equilibrium problem at a particular fixed temperature
* and pressure
*
* ipr = 1 -> Print results to standard output
* 0 -> don't report on anything
* ip1 = 1 -> Print intermediate results.
* maxit -> Maximum number of iterations for the algorithm
* T = Temperature (Kelvin)
* pres = Pressure (pascal)
*
* Return Codes
* ------------------
* 0 = Equilibrium Achieved
* 1 = Range space error encountered. The element abundance criteria are
* only partially satisfied. Specifically, the first NC= (number of
* components) conditions are satisfied. However, the full NE
* (number of elements) conditions are not satisfied. The equilibrium
* condition is returned.
* -1 = Maximum number of iterations is exceeded. Convergence was not
* found.
***************************************************************************/
{
int retn, iconv;
/*
* Store the temperature and pressure in the private global variables
*/
m_temperature = T_arg;
m_pressurePA = pres_arg;
/*
* Evaluate the standard state free energies
* at the current temperatures and pressures.
*/
iconv = vcs_evalSS_TP(ipr, ip1, m_temperature, pres_arg);
/*
* Prepare the problem data:
* ->nondimensionalize the free energies using
* the divisor, R * T
*/
vcs_nondim_TP();
/*
* Prep the fe field
*/
vcs_fePrep_TP();
/*
* Decide whether we need an initial estimate of the solution
* If so, go get one. If not, then
*/
if (m_doEstimateEquil) {
retn = vcs_inest_TP();
if (retn != VCS_SUCCESS) {
plogf("vcs_inest_TP returned a failure flag\n");
}
}
/*
* Solve the problem at a fixed Temperature and Pressure
* (all information concerning Temperature and Pressure has already
* been derived. The free energies are now in dimensionless form.)
*/
iconv = vcs_solve_TP(ipr, ip1, maxit);
/*
* Redimensionalize the free energies using
* the reverse of vcs_nondim to add back units.
*/
vcs_redim_TP();
/*
* Return the convergence success flag.
*/
return iconv;
}
/*****************************************************************************/
/*****************************************************************************/
/*****************************************************************************/
/*ARGSUSED*/
int VCS_SOLVE::vcs_evalSS_TP(int ipr, int ip1, double Temp, double pres)
/**************************************************************************
*
* vcs_evalSS_TP:
*
* IPR = 1 -> Print results to standard output
* 0 -> don't report on anything
* IP1 = 1 -> Print intermediate results.
* T = Temperature (Kelvin)
* Pres = Pressure (Pascal)
*
* Evaluate the standard state free energies at the current temperature
* and pressure. Ideal gas pressure contribution is added in here.
*
***************************************************************************/
{
// int i;
//double R;
/*
* At this level of the program, we are still using values
* for the free energies that have units.
*/
// R = vcsUtil_gasConstant(m_VCS_UnitsFormat);
/*
* We need to special case VCS_UNITS_UNITLESS, here.
* cpc_ts_GStar_calc() returns units of Kelvin. Also, the temperature
* comes into play in calculating the ideal equation of state
* contributions, and other equations of state also. Therefore,
* we will emulate the VCS_UNITS_KELVIN case, here by changing
* the initial gibbs free energy units to Kelvin before feeding
* them to the cpc_ts_GStar_calc() routine. Then, we will revert
* them back to unitless at the end of this routine.
*/
/*
* Loop over the species calculating the standard state Gibbs free
* energies. -> These are energies that only depend upon the Temperature
* and possibly on the pressure (i.e., ideal gas, etc).
*/
// HKM -> We can change this to looks over phases, calling the vcs_VolPhase
// object. Working to get rid of VCS_SPECIES_THERMO object
//for (i = 0; i < m_numSpeciesTot; ++i) {
// VCS_SPECIES_THERMO *spt = SpeciesThermo[i];
// ff[i] = R * spt->GStar_R_calc(i, Temp, pres);
//}
for (size_t iph = 0; iph < m_numPhases; iph++) {
vcs_VolPhase* vph = m_VolPhaseList[iph];
vph->setState_TP(m_temperature, m_pressurePA);
vph->sendToVCS_GStar(VCS_DATA_PTR(m_SSfeSpecies));
}
if (m_VCS_UnitsFormat == VCS_UNITS_UNITLESS) {
for (size_t i = 0; i < m_numSpeciesTot; ++i) {
m_SSfeSpecies[i] /= Temp;
}
}
return VCS_SUCCESS;
} /***************************************************************************/
/*****************************************************************************/
/*****************************************************************************/
/*****************************************************************************/
void VCS_SOLVE::vcs_fePrep_TP(void)
/**************************************************************************
*
*
***************************************************************************/
{
for (size_t i = 0; i < m_numSpeciesTot; ++i) {
/*
* For single species phases, initialize the chemical
* potential with the value of the standard state chemical
* potential. This value doesn't change during the calculation
*/
if (m_SSPhase[i]) {
m_feSpecies_old[i] = m_SSfeSpecies[i];
m_feSpecies_new[i] = m_SSfeSpecies[i];
}
}
} /* vcs_fePrep_TP() ********************************************************/
}