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chemequil.c
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/* ------- file: -------------------------- chemequil.c -------------
Version: rh2.0
Author: Han Uitenbroek (huitenbroek@nso.edu)
Last modified: Mon Apr 18 07:08:41 2011 --
-------------------------- ----------RH-- */
#include <stdlib.h>
#include <math.h>
#include <string.h>
#include "rh.h"
#include "atom.h"
#include "atmos.h"
#include "background.h"
#include "accelerate.h"
#include "constant.h"
#include "error.h"
#include "statistics.h"
#include "inputs.h"
#define COMMENT_CHAR "#"
/* --- Acceleration parameters -- -------------- */
#define NG_CHEM_DELAY 0
#define NG_CHEM_ORDER 0
#define NG_CHEM_PERIOD 0
/* --- Evaluate chemical equilibrium for set of molecules and the complete
and sufficient set of their constituent nuclei.
Equations to solve:
1) Conservation of number density for each constituent:
n_i + Sum_m {N_i^m * n_m} = A_i * nHtot,
n_i are the atomic population number densities (all atoms and ions
of one species not bound in molecules), abund_i the element abundance,
n_m the molecular number densities of molecules containing element i,
and N_i^m is the number of nuclei of element i in molecule m.
2) Chemical equilibrium for each molecule (Saha):
n_m = Prod_i {(f0_i * n_i)^N_i^m} * Phi_m(T),
where f0_i is the fraction of atoms i in the neutral stage,
and Phi_m(T) is the equilibrium constant for molecule m.
If molecule n_m has a charge of +1, one of the f0_i is replaced
by f1_i, the fraction of element i in the first ionization stage.
Note: Molecules with other charge than 0 or +1 are currently not allowed
and are rejected in routine readMolecule.c
-- The Hminus population number is added in the hydrogen conservatiom
equation, which is always the first equation.
Hmin formation is given by:
nHmin = ne * nH * PhiHmin,
where PhiHmin = 1/4 * (h^2/(2PI m_e kT))^3/2 exp(Ediss/kT)
Note: The total hydrogen number density (including protons, H-, and
nuclei that are part of molecules like H2 and H2+ is stored in
atmos->nHtot. The total number not in molecules or H- (i.e. the
neutral atoms plus the protons is stored in atmos->H.ntotal.
Note: Although the partial derivatives matrix df is mostly constant
we have to refill it every iteration since the LU-decomposition
used in the matrix inversion routine uses the matrix as scratch
space. An alternative would be to copy the matrix before inversion.
Note: The following order is used for the number densities in the
Newton-Raphson scheme:
[nH, n_nuclei[1..Nnuclei-1], n_molecules[0..atmos->Nmolecules]]
The equations in the Newton-Raphson scheme are ordered as follows:
- equations for number conservation of nucleus[0..Nnucl-1]
- Saha equations for molecules[0..atmos->Nmolecules]
-- -------------- */
/* --- Function prototypes -- -------------- */
/* --- Global variables -- -------------- */
extern Atmosphere atmos;
extern InputData input;
extern char messageStr[];
/* ------- begin -------------------------- ChemicalEquilibrium.c --- */
void ChemicalEquilibrium(int NmaxIter, double iterLimit)
{
const char routineName[] = "ChemicalEquilibrium";
register int k, i, j, nu;
char tmpStr[7];
bool_t quiet;
int Nequation, **nucl_index, niter, Nnuclei, Ngdelay, Ngperiod,
Ngorder, Nmaxstage;
double *f, *a, *n, **df, *Phi, PhiHmin, fHmin, CI, dnmax = 0.0,
*fn0, fraction, saha, *fjk, *dfjk;
struct Ng *Ngn;
Atom *atom;
Molecule *molecule;
Element **nuclei;
getCPU(3, TIME_START, NULL);
/* --- Constant for Saha equation Hminus -- -------------- */
CI = (HPLANCK/(2.0*PI*M_ELECTRON)) * (HPLANCK/KBOLTZMANN);
/* --- Solve the chemical equilibrium equations. First,
determine for what atoms and molecules the equilibrium
equations have to be solved. -- -------------- */
/* --- Collect pointers to elements that can be bound in molecules. */
Nnuclei = 0;
nuclei = (Element **) malloc(atmos.Nelem * sizeof(Element *));
for (i = 0; i < atmos.Nelem; i++) {
if (atmos.elements[i].Nmolecule > 0) {
nuclei[Nnuclei++] = &atmos.elements[i];
}
}
nuclei = (Element **) realloc(nuclei, Nnuclei * sizeof(Element *));
/* --- Check that first Nucleus is hydrogen -- -------------- */
if (!strstr(nuclei[0]->ID, "H ")) {
sprintf(messageStr, "First nucleus must be H not %s "
"(check H2.molecule)", nuclei[0]->ID);
Error(ERROR_LEVEL_2, routineName, messageStr);
}
Nmaxstage = 0;
for (j = 0; j < Nnuclei; j++) {
if (nuclei[j]->model != NULL) {
if (nuclei[j]->model->stage[0] > 0) {
sprintf(messageStr,
"Model for element %s does not have a neutral stage\n"
" needed for molecular formation\n",
nuclei[j]->ID);
Error(ERROR_LEVEL_2, routineName, messageStr);
}
} else
Nmaxstage = MAX(Nmaxstage, nuclei[j]->Nstage);
}
if (Nmaxstage) {
fjk = (double *) malloc(Nmaxstage * sizeof(double));
dfjk = (double *) malloc(Nmaxstage * sizeof(double));
}
/* --- Quantity nucl_index[i][j] stores the index (in array nuclei)
of the jth element bound in molecule i -- -------------- */
nucl_index = (int **) malloc(atmos.Nmolecule * sizeof(int *));
for (i = 0; i < atmos.Nmolecule; i++) {
molecule = &atmos.molecules[i];
nucl_index[i] = (int *) malloc(molecule->Nelement * sizeof(int));
for (j = 0; j < molecule->Nelement; j++) {
for (nu = 0; nu < Nnuclei; nu++) {
if (nuclei[nu] == &atmos.elements[molecule->pt_index[j]]) {
nucl_index[i][j] = nu;
break;
}
}
}
}
/* --- Number of equations -- -------------- */
Nequation = Nnuclei + atmos.Nmolecule;
/* --- Allocate temporary storage space.
Quantities for the Newton Raphson -- -------------- */
f = (double *) malloc(Nequation * sizeof(double));
n = (double *) calloc(Nequation, sizeof(double));
df = matrix_double(Nequation, Nequation);
a = (double *) calloc(Nequation, sizeof(double));
/* --- Equilibrium constant for each molecule, and neutral
fraction for each nucleus -- -------------- */
Phi = (double *) malloc(atmos.Nmolecule * sizeof(double));
fn0 = (double *) malloc(Nnuclei * sizeof(double));
/* --- Initialize structure for Ng convergence acceleration -- ---- */
Ngn = NgInit(Nequation, Ngdelay=NG_CHEM_DELAY,
Ngorder=NG_CHEM_ORDER, Ngperiod=NG_CHEM_PERIOD, n);
/* --- Go through spatial grid and solve (local) equations -- ----- */
for (k = 0; k < atmos.Nspace; k++) {
/* --- Collect for each atom the population fraction of
the neutral stage -- -------------- */
for (i = 0; i < Nnuclei; i++) {
if ((atom = nuclei[i]->model) == NULL) {
/* --- If no atomic model is present for this nucleus -- ---- */
getfjk(nuclei[i], atmos.ne[k], k, fjk, dfjk);
fn0[i] = fjk[0];
a[i] = nuclei[i]->abund * atmos.nHtot[k];
} else {
/* --- Atomic model has been read for this nucleus -- ------- */
fn0[i] = 0.0;
for (j = 0; j < atom->Nlevel; j++) {
if (atom->stage[j] > 0) break;
if (atom->active &&
atom->initial_solution != OLD_POPULATIONS)
fn0[i] += atom->nstar[j][k];
else
fn0[i] += atom->n[j][k];
}
fn0[i] /= atom->ntotal[k];
a[i] = atom->abundance * atmos.nHtot[k];
}
}
PhiHmin = 0.25*pow(CI/atmos.T[k], 1.5) *
exp(E_ION_HMIN / (KBOLTZMANN * atmos.T[k]));
fHmin = atmos.ne[k] * fn0[0]*PhiHmin;
/* --- Equilibrium constant for each molecule at this location -- */
for (i = 0; i < atmos.Nmolecule; i++)
Phi[i] = equilconstant(&atmos.molecules[i], atmos.T[k]);
/* --- Initial solution of atomic number densities, and
the molecules. Assume everything is dissociated -- ------- */
for (i = 0; i < Nnuclei; i++) n[i] = a[i];
for (i = 0; i < atmos.Nmolecule; i++) n[Nnuclei+i] = 0.0;
/* --- Reset counter in Ng structure, store initial solution - -- */
Ngn->count = 1;
for (i = 0; i < Nequation; i++) Ngn->previous[0][i] = n[i];
/* --- Iterate to convergence, with maximum number NmaxIter -- -- */
niter = 1;
while (niter <= NmaxIter) {
for (i = 0; i < Nequation; i++) {
f[i] = n[i] - a[i];
for (j = 0; j < Nequation; j++) df[i][j] = 0.0;
df[i][i] = 1.0;
}
/* --- Add nHminus to the H number conservation equation -- --- */
f[0] += fHmin * n[0];
df[0][0] += fHmin;
/* --- Fill in the rest of the population matrix f[] and its
derivative df[][] -- -------------- */
for (i = 0; i < atmos.Nmolecule; i++) {
molecule = &atmos.molecules[i];
saha = Phi[i];
for (j = 0; j < molecule->Nelement; j++) {
nu = nucl_index[i][j];
saha *= pow(fn0[nu] * n[nu], molecule->pt_count[j]);
/* --- Contributions to equation of conservation for the
nuclei in this molecule -- -------------- */
f[nu] += molecule->pt_count[j] * n[Nnuclei + i];
}
/* --- Saha equation for this molecule -- -------------- */
saha /= pow(atmos.ne[k], molecule->charge);
f[Nnuclei + i] -= saha;
/* --- Fill the derivatives matrix -- -------------- */
for (j = 0; j < molecule->Nelement; j++) {
nu = nucl_index[i][j];
df[nu][Nnuclei + i] += molecule->pt_count[j];
df[Nnuclei + i][nu] = -saha * (molecule->pt_count[j]/n[nu]);
}
}
/* --- Solve linearized equations -- -------------- */
SolveLinearEq(Nequation, df, f, TRUE);
for (i = 0; i < Nequation; i++) n[i] -= f[i];
/* --- Check convergence and accelerate if appropriate -- ----- */
Accelerate(Ngn, n);
sprintf(messageStr,
"\n%s-- Chemical equilibrium: depth %3.3d, iteration %d",
(niter == 1) ? "\n" : "", k, niter);
if ((dnmax = MaxChange(Ngn, messageStr, quiet=TRUE)) <= iterLimit)
break;
niter++;
}
if (dnmax > iterLimit) {
sprintf(messageStr, "Iteration not converged:\n"
" temperature: %6.1f [K], \n"
" density: %9.3E [m^-3],\n dnmax: %9.3E\n",
atmos.T[k], atmos.nHtot[k], dnmax);
Error(WARNING, "ChemicalEquilibrium", messageStr);
}
/* --- Store population numbers nuclei -- -------------- */
for (i = 0; i < Nnuclei; i++) {
if ((atom = nuclei[i]->model) != NULL) {
fraction = n[i] / atom->ntotal[k];
for (j = 0; j < atom->Nlevel; j++) {
atom->nstar[j][k] *= fraction;
if (atom->n != atom->nstar) atom->n[j][k] *= fraction;
}
atom->ntotal[k] = n[i];
}
}
/* --- Store Hmin density -- -------------- */
atmos.nHmin[k] = atmos.ne[k] * (n[0] * PhiHmin);
/* --- Store molecular densities -- -------------- */
for (i = 0; i < atmos.Nmolecule; i++)
atmos.molecules[i].n[k] = n[Nnuclei + i];
}
/* --- Check whether active atom, if present, is in list of nuclei.
If so print out a warning -- -------------- */
for (nu = 0; nu < Nnuclei; nu++) {
atom = nuclei[nu]->model;
if (atom && atom->active) {
sprintf(messageStr, "\nReduced number density of"
" active atom %s due to molecule%s\n ",
atom->ID, (nuclei[nu]->Nmolecule > 1) ? "s" : "");
for (i = 0; i < nuclei[nu]->Nmolecule; i++) {
sprintf(tmpStr, "%s%s",
atmos.molecules[nuclei[nu]->mol_index[i]].ID,
(i == nuclei[nu]->Nmolecule - 1) ? "\n\n" : ", ");
strcat(messageStr, tmpStr);
}
Error(MESSAGE, routineName, messageStr);
}
}
/* --- Clean up -- -------------- */
free(f); free(n); free(a);
free(Phi); free(fn0);
freeMatrix((void **) df);
NgFree(Ngn);
free(nuclei);
for (i = 0; i < atmos.Nmolecule; i++) free(nucl_index[i]);
free(nucl_index);
if (Nmaxstage) {
free(fjk);
free(dfjk);
}
getCPU(3, TIME_POLL, "Chemical equilibrium");
}
/* ------- end ---------------------------- ChemicalEquilibrium.c --- */
/* ------- begin -------------------------- partfunction.c ---------- */
double partfunction(struct Molecule *molecule, double T)
{
register int i;
double pf = 0.0, t;
if (T < molecule->Tmin || T > molecule->Tmax)
return pf;
/* --- Evaluate polynomial in temperature for partition function -- */
switch (molecule->fit) {
case KURUCZ_70:
pf = molecule->pf_coef[0];
for (i = 1; i < molecule->Npf; i++)
pf = pf*T + molecule->pf_coef[i];
pf = exp(pf);
break;
case KURUCZ_85:
t = T * 1.0E-4;
pf = molecule->pf_coef[0];
for (i = 1; i < molecule->Npf; i++)
pf = pf*t + molecule->pf_coef[i];
pf = exp(pf);
break;
case SAUVAL_TATUM_84:
t = log10(THETA0 / T);
pf = molecule->pf_coef[0];
for (i = 1; i < molecule->Npf; i++)
pf = pf*t + molecule->pf_coef[i];
pf = POW10(pf);
break;
case IRWIN_81:
t = log(T);
pf = molecule->pf_coef[0];
for (i = 1; i < molecule->Npf; i++)
pf = pf*t + molecule->pf_coef[i];
pf = exp(pf);
break;
case TSUJI_73:
break;
default:
sprintf(messageStr,
"Unknown method for calculation of partition function\n"
"for molecule %s: %d", molecule->ID, molecule->fit);
Error(ERROR_LEVEL_2, "partfunction", messageStr);
}
return pf;
}
/* ------- end ---------------------------- partfunction.c ---------- */
/* ------- begin -------------------------- equilconstant.c --------- */
double equilconstant(struct Molecule *molecule, double T)
{
register int i;
int mk;
double kT, t, eqc = 0.0, theta, cgs_to_SI = 1.0;
if (T < molecule->Tmin || T > molecule->Tmax)
return eqc;
/* --- Evaluate polynomial in temperature for equilibrium constant.
Constant should have units of [m^3,6,9, etc] -- ------------ */
switch (molecule->fit) {
case KURUCZ_70:
kT = KBOLTZMANN * T;
mk = molecule->Nnuclei - 1 - molecule->charge;
eqc = molecule->eqc_coef[0];
for (i = 1; i < molecule->Neqc; i++)
eqc = eqc*T + molecule->eqc_coef[i];
eqc = exp(molecule->Ediss/kT + eqc - 1.5*mk*log(T));
cgs_to_SI = pow(CUBE(CM_TO_M), mk);
break;
case KURUCZ_85:
t = T * 1.0E-4;
kT = KBOLTZMANN * T;
mk = molecule->Nnuclei - 1 - molecule->charge;
eqc = molecule->eqc_coef[0];
for (i = 1; i < molecule->Neqc; i++)
eqc = eqc*t + molecule->eqc_coef[i];
eqc = exp(molecule->Ediss/kT + eqc - 1.5*mk*log(T));
cgs_to_SI = pow(CUBE(CM_TO_M), mk);
break;
case IRWIN_81:
/* ---- Use SAUVAL_TATUM_84 for equilibrium constant -- ---------- */
;
case SAUVAL_TATUM_84:
theta = THETA0 / T;
t = log10(theta);
kT = KBOLTZMANN * T;
eqc = molecule->eqc_coef[0];
for (i = 1; i < molecule->Neqc; i++)
eqc = eqc*t + molecule->eqc_coef[i];
eqc = POW10((molecule->Ediss/EV) * theta - eqc) * kT;
/* --- Constants are already given in SI units by Sauval & Tatum - */
cgs_to_SI = 1.0;
break;
case TSUJI_73:
theta = THETA0 / T;
kT = KBOLTZMANN * T;
eqc = molecule->eqc_coef[0];
for (i = 1; i < molecule->Neqc; i++)
eqc = eqc*theta + molecule->eqc_coef[i];
eqc = SQ(kT) * POW10(-eqc);
cgs_to_SI = pow(CUBE(CM_TO_M) / ERG_TO_JOULE, molecule->Nnuclei-1);
break;
default:
sprintf(messageStr,
"Unknown method for calculation of equilibrium constant\n"
"for molecule %s: %d", molecule->ID, molecule->fit);
Error(ERROR_LEVEL_2, "equilconstant", messageStr);
}
return eqc * cgs_to_SI;
}
/* ------- end ---------------------------- equilconstant.c --------- */