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/* This file is part of Cloudy and is copyright (C)1978-2008 by Gary J. Ferland and
 * others.  For conditions of distribution and use see copyright notice in license.txt */
/*GrainMakeDiffuse main routine for generating the grain diffuse emission, called by RT_diffuse */
#include "cddefines.h"
#include "physconst.h"
#include "rfield.h"
#include "phycon.h"
#include "dense.h"
#include "hmi.h"
#include "thermal.h"
#include "trace.h"
#include "thirdparty.h"
#include "iterations.h"
#include "grainvar.h"
#include "grains.h"

#define NO_ATOMS(ND) (gv.bin[ND]->AvVol*gv.bin[ND]->dustp[0]/ATOMIC_MASS_UNIT/gv.bin[ND]->atomWeight)

/* NB NB -- the sequence below has been carefully chosen and should NEVER be
 *          altered unless you really know what you are doing !! */
/* >>chng 03 jan 16, introduced QH_THIGH_FAIL and started using splint_safe and spldrv_safe
 *                   throughout the code; this solves the parispn_a031_sil.in bug, PvH */
/* >>chng 03 jan 16, rescheduled QH_STEP_FAIL as non-fatal; it can be triggered at very low temps, PvH */
typedef enum {
        /* the following are OK */
        /* 0        1               2              3    */
        QH_OK, QH_ANALYTIC, QH_ANALYTIC_RELAX, QH_DELTA, 
        /* the following are mild errors we already recovered from */
        /*     4              5              6             7        */
        QH_NEGRATE_FAIL, QH_LOOP_FAIL, QH_ARRAY_FAIL, QH_THIGH_FAIL,
        /* any of these errors will prompt qheat to do another iteration */
        /*  8          9             10             11       */
        QH_RETRY, QH_CONV_FAIL, QH_BOUND_FAIL, QH_DELTA_FAIL,
        /* any error larger than QH_NO_REBIN will cause GetProbDistr_LowLimit to return
         * before even attempting to rebin the results; we may be able to recover though... */
        /*   12          13            14            15       */
        QH_NO_REBIN, QH_LOW_FAIL, QH_HIGH_FAIL, QH_STEP_FAIL,
        /* any case larger than QH_FATAL is truly pathological; there is no hope of recovery */
        /* 16          17           18             19      */
        QH_FATAL, QH_WIDE_FAIL, QH_NBIN_FAIL, QH_REBIN_FAIL
} QH_Code;

/*================================================================================*/
/* definitions relating to quantum heating routines */

/* this is the minimum number of bins for quantum heating calculation to be valid */
static const long NQMIN = 10L;

/* this is the lowest value for dPdlnT that should be included in the modeling */
static const double PROB_CUTOFF_LO = 1.e-15;
static const double PROB_CUTOFF_HI = 1.e-20;
static const double SAFETY = 1.e+8;

/* during the first NSTARTUP steps, use special algorithm to calculate stepsize */
static const long NSTARTUP = 5L;

/* if the average number of multiple events is above this number
 * don't try full quantum heating treatment. */
static const double MAX_EVENTS = 150.;

/* maximum number of tries for quantum heating routine */
/* >>chng 02 jan 30, changed LOOP_MAX from 10 -> 20, PvH */
static const long LOOP_MAX = 20L;

/* if all else fails, divide temp estimate by this factor */
static const double DEF_FAC = 3.;

/* total probability for all bins should not deviate more than this from 1. */
static const double PROB_TOL = 0.02;

/* after NQTEST steps, make an estimate if prob distr will converge in NQGRID steps */
/* >>chng 02 jan 30, change NQTEST from 1000 -> 500, PvH */
static const long NQTEST = 500L;

/* if the ratio fwhm/Umax is lower than this number
 * don't try full quantum heating treatment. */
static const double FWHM_RATIO = 0.1;
/* if the ratio fwhm/Umax is lower than this number
 * don't even try analytic approximation, use delta function instead */
static const double FWHM_RATIO2 = 0.007;

/* maximum number of steps for integrating quantum heating probability distribution */
static const long MAX_LOOP = 2*NQGRID;

/* this is the tolerance used while integrating the temperature distribution of the grains */
static const double QHEAT_TOL = 5.e-3;

/* maximum number of tries before we declare that probability distribution simply won't fit */
static const long WIDE_FAIL_MAX = 3;

/* multipliers for PROB_TOL used in GetProbDistr_HighLimit */
static const double STRICT = 1.;
static const double RELAX = 15.;

/* when rebinning quantum heating results, make ln(qtemp[i]/qtemp[i-1]) == QT_RATIO */
/* this constant determines the accuracy with which the Wien tail of the grain emission
 * is calculated; if x = h*nu/k*T_gr and d = QT_RATIO-1., then the relative accuracy of
 * the flux in the Wien tail is Acc = fabs(x*d^2/12 - x^2*d^2/24). A typical value of x
 * would be x = 15, so QT_RATIO = 1.03 should converge the spectrum to better than 1% */
static const double QT_RATIO = 1.03;


/*================================================================================*/
/* global variables */

/* these data define the enthalpy function for silicates
 * derived from:
 * >>refer      grain   physics Guhathakurta & Draine, 1989, ApJ, 345, 230
 * coefficients converted to rydberg energy units, per unit atom
 * assuming a density of 3.3 g/cm^3 and pure MgSiFeO4.
 * this is not right, but the result is correct because number
 * of atoms will be calculated using the same assumption. */

/* this is the specific density of silicate in g/cm^3 */
static const double DEN_SIL = 3.30;

/* these are the mean molecular weights per atom for MgSiFeO4 and SiO2 in amu */
static const double MW_SIL = 24.6051;
/*#define MW_SIO2     20.0283*/

static const double tlim[5]={0.,50.,150.,500.,DBL_MAX};
static const double ppower[4]={2.00,1.30,0.68,0.00};
static const double cval[4]={
        1.40e3/DEN_SIL*ATOMIC_MASS_UNIT*MW_SIL/EN1RYD,
        2.20e4/DEN_SIL*ATOMIC_MASS_UNIT*MW_SIL/EN1RYD,
        4.80e5/DEN_SIL*ATOMIC_MASS_UNIT*MW_SIL/EN1RYD,
        3.41e7/DEN_SIL*ATOMIC_MASS_UNIT*MW_SIL/EN1RYD};


/* initialize phiTilde */
STATIC void qheat_init(long,/*@out@*/double[],/*@out@*/double*);
/* worker routine, this implements the algorithm of Guhathakurtha & Draine */
STATIC void GetProbDistr_LowLimit(long,double,double,double,/*@in@*/double[],/*@in@*/double[],
                                  /*@out@*/double[],/*@out@*/double[],/*@out@*/double[],
                                  /*@out@*/long*,/*@out@*/double*,long*,/*@out@*/QH_Code*);
/* try two consecutive integration steps using stepsize "step/2." (yielding p[k]),
 * and also one double integration step using stepsize "step" (yielding p2k). */
STATIC double TryDoubleStep(double[],double[],double[],double[],double[],double[],
                            double[],double,/*@out@*/double*,long,long,/*@out@*/bool*);
/* calculate logarithmic integral from (x1,y1) to (x2,y2) */
STATIC double log_integral(double,double,double,double);
/* scan the probability distribution for valid range */
STATIC void ScanProbDistr(double[],double[],long,double,long,double,/*@out@*/long*,/*@out@*/long*,
                          /*@out@*/long*,long*,QH_Code*);
/* rebin the quantum heating results to speed up RT_diffuse */
STATIC long RebinQHeatResults(long,long,long,double[],double[],double[],double[],double[],
                              double[],double[],QH_Code*);
/* calculate approximate probability distribution in high intensity limit */
STATIC void GetProbDistr_HighLimit(long,double,double,double,/*@out@*/double[],/*@out@*/double[],
                                   /*@out@*/double[],/*@out@*/double*,/*@out@*/long*,
                                   /*@out@*/double*,/*@out@*/QH_Code*);
/* derivative of the enthalpy function dU/dT */
STATIC double uderiv(double,long);
/* enthalpy function */
STATIC double ufunct(double,long,/*@out@*/bool*);
/* inverse enthalpy function */
STATIC double inv_ufunct(double,long,/*@out@*/bool*);
/* helper function for calculating enthalpy, uses Debye theory */
STATIC double DebyeDeriv(double,long);

/* >>chng 01 oct 29, introduced gv.bin[nd]->cnv_H_pGR, cnv_GR_pH, etc. PvH */


/* main routine for generating the grain diffuse emission, called by RT_diffuse */
void GrainMakeDiffuse(void)
{
        long i,
          j,
          nd;
        double bfac,
          f,
          factor,
          flux,
          x;

        /* >>chng 01 sep 11, replace array allocation on stack with
         * MALLOC to avoid bug in gcc 3.0 on Sparc platforms, PvH */
        double *qtemp/*[NQGRID]*/, *qprob/*[NQGRID]*/;

#       ifndef NDEBUG
        bool lgNoTdustFailures;
        double BolFlux,
          Comparison1,
          Comparison2;
#       endif

        /* this assures 6-digit precision in the evaluation of the exponential below */
        const double LIM1 = pow(2.e-6,1./2.);
        const double LIM2 = pow(6.e-6,1./3.);

        DEBUG_ENTRY( "GrainMakeDiffuse()" );

        factor = 2.*PI4*POW2(FR1RYD/SPEEDLIGHT)*FR1RYD;
        /* >>chng 96 apr 26 upper limit chng from 15 to 75 Peter van Hoof  */
        /* >>chng 00 apr 10 use constants appropriate for double precision, by PvH */
        x = log(0.999*DBL_MAX);

        /* save grain emission per unit volume */
        for( i=0; i < rfield.nflux; i++ )
        {
                /* used in RT_diffuse to derive total emission */
                gv.GrainEmission[i] = 0.;
                gv.SilicateEmission[i] = 0.;
                gv.GraphiteEmission[i] = 0.;
        }

        qtemp = (double*)MALLOC((size_t)(NQGRID*sizeof(double)));
        qprob = (double*)MALLOC((size_t)(NQGRID*sizeof(double)));

        for( nd=0; nd < gv.nBin; nd++ )
        {
                strg_type scase;
                bool lgLocalQHeat;
                long qnbin=-200;
                realnum *grn, threshold;
                double xx;

                /* save emission from this species */
                scase = gv.which_strg[gv.bin[nd]->matType];
                switch( scase )
                {
                case STRG_SIL:
                        grn = gv.SilicateEmission;
                        break;
                case STRG_CAR:
                        grn = gv.GraphiteEmission;
                        break;
                default:
                        fprintf( ioQQQ, " GrainMakeDiffuse called with unknown storage class: %d\n", scase );
                        cdEXIT(EXIT_FAILURE);
                }

                /* this local copy is necessary to keep lint happy */
                lgLocalQHeat = gv.bin[nd]->lgQHeat;
                /* >>chng 04 nov 09, do not evaluate quantum heating if abundance is negligible, PvH
                 * this prevents PAH's deep inside molecular regions from failing if GrnVryDepth is used */
                /* >>chng 04 dec 31, introduced separate thresholds near I-front and in molecular region, PvH */
                threshold = ( dense.xIonDense[ipHYDROGEN][0]+dense.xIonDense[ipHYDROGEN][1] > hmi.H2_total ) ?
                        gv.dstAbundThresholdNear : gv.dstAbundThresholdFar;

                if( lgLocalQHeat && gv.bin[nd]->dstAbund >= threshold )
                {
                        qheat(qtemp,qprob,&qnbin,nd);

                        if( gv.bin[nd]->lgUseQHeat )
                        {
                                ASSERT( qnbin > 0 );
                        }
                }
                else
                {
                        /* >> chng 04 dec 31, repaired bug lgUseQHeat not set when abundance below threshold, PvH */
                        gv.bin[nd]->lgUseQHeat = false;
                }

                flux = 1.;
                /* flux can only become zero in the Wien tail */
                /* >>chng 04 jan 25, replaced flux > 0. with (realnum)flux > 0.f, PvH */
                for( i=0; i < rfield.nflux && (realnum)flux > 0.f; i++ )
                {
                        flux = 0.;
                        if( lgLocalQHeat && gv.bin[nd]->lgUseQHeat )
                        {
                                xx = 1.;
                                /* we start at high temperature end and work our way down
                                 * until contribution becomes negligible */
                                for( j=qnbin-1; j >= 0 && xx > flux*DBL_EPSILON; j-- )
                                {
                                        f = TE1RYD/qtemp[j]*rfield.anu[i];
                                        if( f < x )
                                        {
                                                /* want the number exp(hnu/kT) - 1, two expansions */
                                                /* >>chng 04 jan 25, changed 1.e-5 -> LIM1, LIM2, PvH */
                                                if( f > LIM2 )
                                                        bfac = exp(f) - 1.;
                                                else if( f > LIM1 )
                                                        bfac = (1. + 0.5*f)*f;
                                                else
                                                        bfac = f;
                                                xx = qprob[j]*gv.bin[nd]->dstab1[i]*rfield.anu2[i]*
                                                        rfield.widflx[i]/bfac;
                                                flux += xx;
                                        }
                                        else
                                        {
                                                xx = 0.;
                                        }
                                }
                        }
                        else
                        {
                                f = TE1RYD/gv.bin[nd]->tedust*rfield.anu[i];
                                if( f < x )
                                {
                                        /* >>chng 04 jan 25, changed 1.e-5 -> LIM1, LIM2, PvH */
                                        if( f > LIM2 )
                                                bfac = exp(f) - 1.;
                                        else if( f > LIM1 )
                                                bfac = (1. + 0.5*f)*f;
                                        else
                                                bfac = f;
                                        flux = gv.bin[nd]->dstab1[i]*rfield.anu2[i]*rfield.widflx[i]/bfac;
                                }
                        }

                        /* do multiplications outside loop, PvH */
                        flux *= factor*gv.bin[nd]->cnv_H_pCM3;

                        /* remember local emission these are zeroed out on each zone 
                         * above, and now incremented so is unit emission from this zone */
                        gv.GrainEmission[i] += (realnum)flux;
                        /* unit emission for each different grain type */
                        grn[i] += (realnum)flux;
                }
        }

        free( qprob );
        free( qtemp );

#       ifndef NDEBUG
        /*********************************************************************************
         *
         * Following are three checks on energy and charge conservation by the grain code.
         * Their primary function is as an internal consistency check, so that coding
         * errors get caught as early as possible. This is why the program terminates as
         * soon as any one of the checks fails.
         *
         * NB NB - despite appearances, these checks do NOT guarantee overall energy
         *         conservation in the Cloudy model to the asserted tolerance, see note 1B !
         *
         * Note 1: there are two sources for energy imbalance in the grain code (see A & B).
         *   A: Interpolation in dstems. The code calculates how much energy the grains
         *      emit in thermal radiation (gv.bin[nd]->GrainHeat), and converts that into
         *      an (average) grain temperature by reverse interpolation in dstems. If
         *      quantum heating is not used, that temperature is used directly to generate
         *      the local diffuse emission. Hence the finite resolution of the dstems grid
         *      can lead to small errors in flux. This is tested in Check 1. The maximum
         *      error of interpolating in dstems scales with NDEMS^-3. The same problem
         *      can also occur when quantum heating is used, however, the fact that many
         *      bins are used will probably lead to a cancellation effect of the errors.
         *   B: RT_OTS_Update gets called AFTER grain() has completed, so the grain heating
         *      was calculated using a different version of the OTS fields than the one
         *      that gets fed into the RT routines (where the actual attenuation of the
         *      radiation fields by the grain opacity is done). This can lead to an energy
         *      imbalance, depending on how accurate the convergence of the OTS fields is.
         *      This is outside the control of the grain code and is therefore NOT checked.
         *      Rather, the grain code remembers the contribution from the old OTS fields
         *      (through gv.bin[nd]->BolFlux) and uses that in Check 3. In most models the
         *      difference will be well below 0.1%, but in AGN type models where OTS continua
         *      are important, the energy imbalance can be of the order of 0.5% of the grain
         *      heating (status nov 2001). On 04 jan 25 the initialization of phiTilde has
         *      been moved to qheat, implying that phiTilde now uses the updated version of
         *      the OTS fields. The total amount of radiated energy however is still based
         *      on gv.bin[nd]->GrainHeat which uses the old version of the OTS fields.
         *   C: Energy conservation for collisional processes is guaranteed by adding in
         *      (very small) correction terms. These corrections are needed to cover up
         *      small imperfection in the theory, and cannot be avoided without making the
         *      already very complex theory even more complex.
         *   D: Photo-electric heating and collisional cooling can have an important effect
         *      on the total heating balance of the gas. Both processes depend strongly on
         *      the grain charge, so assuring proper charge balance is important as well.
         *      This is tested in Check 2.
         *
         * Note 2: for quantum heating it is important to resolve the Maxwell distribution
         *   of the electrons and ions far enough into the tail that the total amount of
         *   energy contained in the remaining tail is negligible. If this is not the case,
         *   the assert at the beginning of the qheat() routine will fail. This is because
         *   the code filling up the phiTilde array in GrainCollHeating() assumes a value for
         *   the average particle energy based on a Maxwell distribution going to infinity.
         *   If the maximum energy used is too low, the assumed average energy would be
         *   incorrect.
         *
         *********************************************************************************/

        lgNoTdustFailures = true;
        for( nd=0; nd < gv.nBin; nd++ )
        {
                if( !gv.bin[nd]->lgTdustConverged )
                {
                        lgNoTdustFailures = false;
                        break;
                }
        }

        /* CHECK 1: does the grain thermal emission conserve energy ? */
        BolFlux = 0.;
        for( i=0; i < rfield.nflux; i++ )
        {
                BolFlux += gv.GrainEmission[i]*rfield.anu[i]*EN1RYD;
        }
        Comparison1 = 0.;
        for( nd=0; nd < gv.nBin; nd++ )
        {
                if( gv.bin[nd]->tedust < gv.bin[nd]->Tsublimat )
                        Comparison1 += CONSERV_TOL*gv.bin[nd]->GrainHeat;
                else
                        /* for high temperatures the interpolation in dstems
                         * is less accurate, so we have to be more lenient */
                        Comparison1 += 10.*CONSERV_TOL*gv.bin[nd]->GrainHeat;
        }

        /* >>chng 04 mar 11, add constant grain temperature to pass assert */
        /* >>chng 04 jun 01, deleted test for constant grain temperature, PvH */
        ASSERT( fabs(BolFlux-gv.GrainHeatSum) < Comparison1 );

        /* CHECK 2: assert charging balance */
        for( nd=0; nd < gv.nBin; nd++ )
        {
                if( gv.bin[nd]->lgChrgConverged )
                {
                        double ave = 0.5*(gv.bin[nd]->RateDn+gv.bin[nd]->RateUp);
                        /* >>chng 04 dec 16, add lgAbort - do not throw assert if we are in 
                         * process of aborting */
                        ASSERT( lgAbort || fabs(gv.bin[nd]->RateDn-gv.bin[nd]->RateUp) < CONSERV_TOL*ave );
                }
        }

        if( lgNoTdustFailures && gv.lgDHetOn && gv.lgDColOn && thermal.ConstGrainTemp == 0. )
        {
                /* CHECK 3: calculate the total energy donated to grains, must be balanced by
                 * the energy emitted in thermal radiation plus various forms of gas heating */
                Comparison1 = 0.;
                for( nd=0; nd < gv.nBin; nd++ )
                {
                        Comparison1 += gv.bin[nd]->BolFlux;
                }
                /* add in collisional heating of grains by plasma (if positive) */
                Comparison1 += MAX2(gv.GasCoolColl,0.);
                /* add in net amount of chemical energy donated by recombining ions and molecule formation */
                Comparison1 += gv.GrainHeatChem;

                /*              thermal emis        PE effect          gas heating by coll    thermionic emis */
                Comparison2 = gv.GrainHeatSum+thermal.heating[0][13]+thermal.heating[0][14]+thermal.heating[0][25];

                /* >>chng 06 jun 02, add test on gv.GrainHeatScaleFactor so that assert not thrown
                 * when set grain heat command is used */
                ASSERT( lgAbort || gv.GrainHeatScaleFactor != 1.f || gv.lgBakesPAH_heat ||
                        fabs(Comparison1-Comparison2)/Comparison2 < CONSERV_TOL );
        }
#       endif
        return;
}


/****************************************************************************
 *
 * qheat: driver routine for non-equilibrium heating of grains
 *
 * This routine calls GetProbDistr_LowLimit, GetProbDistr_HighLimit
 * (which do the actual non-equilibrium calculations), and does the
 * subsequent quality control.
 *
 * Written by Peter van Hoof (UK, CITA, QUB).
 *
 ****************************************************************************/

/* this is the new version of the quantum heating code, used starting Cloudy 96 beta 3 */

void qheat(/*@out@*/ double qtemp[],  /* qtemp[NQGRID] */
           /*@out@*/ double qprob[],  /* qprob[NQGRID] */
           /*@out@*/ long int *qnbin,
           long int nd)
{
        bool lgBoundErr,
          lgDelta,
          lgNegRate,
          lgOK,
          lgTried;
        long int i,
          nWideFail;
        QH_Code ErrorCode,
          ErrorCode2,
          ErrorStart;
        double c0,
          c1,
          c2,
          check,
          DefFac,
          deriv,
          *dPdlnT/*[NQGRID]*/,
          fwhm,
          FwhmRatio,
          integral,
          minBracket,
          maxBracket,
          new_tmin,
          NumEvents,
          oldy,
          *Phi/*[NC_ELL]*/,
          *PhiDrv/*[NC_ELL]*/,
          *phiTilde/*[NC_ELL]*/,
          rel_tol,
          Tmax,
          tol,
          Umax,
          xx,
          y;


        DEBUG_ENTRY( "qheat()" );

        /* sanity checks */
        ASSERT( gv.bin[nd]->lgQHeat );
        ASSERT( nd >= 0 && nd < gv.nBin );

        if( trace.lgTrace && trace.lgDustBug )
        {
                fprintf( ioQQQ, "\n >>>>qheat called for grain %s\n", gv.bin[nd]->chDstLab );
        }

        /* >>chng 01 aug 22, allocate space */
        /* phiTilde is continuum corrected for photo-electric effect, in events/H/s/cell, default depl */
        phiTilde = (double*)MALLOC((size_t)((unsigned)rfield.nupper*sizeof(double)) );
        Phi = (double*)MALLOC((size_t)((unsigned)rfield.nupper*sizeof(double)) );
        PhiDrv = (double*)MALLOC((size_t)((unsigned)rfield.nupper*sizeof(double)) );
        dPdlnT = (double*)MALLOC((size_t)(NQGRID*sizeof(double)) );

        qheat_init( nd, phiTilde, &check );

        check += gv.bin[nd]->GrainHeatColl-gv.bin[nd]->GrainCoolTherm;

        xx = integral = 0.;
        c0 = c1 = c2 = 0.;
        lgNegRate = false;
        oldy = 0.;
        tol = 1.;

        /* >>chng 01 nov 29, rfield.nflux -> gv.qnflux, PvH */
        /* >>chng 03 jan 26, gv.qnflux -> gv.bin[nd]->qnflux, PvH */
        for( i=gv.bin[nd]->qnflux-1; i >= 0; i-- )
        {
                /* >>chng 97 jul 17, to summed continuum */
                /* >>chng 00 mar 30, to phiTilde, to keep track of photo-electric effect and collisions, by PvH */
                /* >>chng 01 oct 10, use trapezoidal rule for integrating Phi, reverse direction of integration.
                 * Phi[i] is now integral from exactly rfield.anu[i] to infinity to second-order precision, PvH */
                /* >>chng 01 oct 30, change normalization of Phi, PhiDrv from <unit>/cm^3 -> <unit>/grain, PvH */
                double fac = ( i < gv.bin[nd]->qnflux-1 ) ? 1./rfield.widflx[i] : 0.;
                /* phiTilde has units events/H/s, y has units events/grain/s/Ryd */
                y = phiTilde[i]*gv.bin[nd]->cnv_H_pGR*fac;
                /* PhiDrv[i] = (Phi[i+1]-Phi[i])/(anu[i+1]-anu[i]), units events/grain/s/Ryd */
                PhiDrv[i] = -0.5*(y + oldy);
                /* there is a minus sign here because we are integrating from infinity downwards */
                xx -= PhiDrv[i]*(rfield.anu[i+1]-rfield.anu[i]);
                /* Phi has units events/grain/s */
                Phi[i] = xx;

#               ifndef NDEBUG
                /* trapezoidal rule is not needed for integral, this is also second-order correct */
                integral += phiTilde[i]*gv.bin[nd]->cnv_H_pCM3*rfield.anu[i]*EN1RYD;
#               endif

                /* c<n> has units Ryd^(n+1)/grain/s */
                c0 += Phi[i]*rfield.widflx[i];
                c1 += Phi[i]*rfield.anu[i]*rfield.widflx[i];
                c2 += Phi[i]*POW2(rfield.anu[i])*rfield.widflx[i];

                lgNegRate = lgNegRate || ( phiTilde[i] < 0. );

                oldy = y;
        }

        /* sanity check */
        ASSERT( fabs(check-integral)/check <= CONSERV_TOL );

#       if 0
        {
                char fnam[50];
                FILE *file;

                sprintf(fnam,"Lambda_%2.2ld.asc",nd);
                file = fopen(fnam,"w");
                for( i=0; i < NDEMS; ++i )
                        fprintf(file,"%e %e %e\n",
                                exp(gv.dsttmp[i]),
                                ufunct(exp(gv.dsttmp[i]),nd,&lgBoundErr),
                                exp(gv.bin[nd]->dstems[i])*gv.bin[nd]->cnv_H_pGR/EN1RYD);
                fclose(file);

                sprintf(fnam,"Phi_%2.2ld.asc",nd);
                file = fopen(fnam,"w");
                for( i=0; i < gv.bin[nd]->qnflux; ++i )
                        fprintf(file,"%e %e\n", rfield.anu[i],Phi[i]);
                fclose(file);
        }
#       endif

        /* Tmax is where p(U) will peak (at least in high intensity limit) */
        Tmax = gv.bin[nd]->tedust;
        /* grain enthalpy at peak of p(U), in Ryd */
        Umax = ufunct(Tmax,nd,&lgBoundErr);
        ASSERT( !lgBoundErr ); /* this should never happen */
        /* y is dln(Lambda)/dlnT at Tmax */
        spldrv_safe(gv.dsttmp,gv.bin[nd]->dstems,gv.bin[nd]->dstslp2,NDEMS,log(Tmax),&y,&lgBoundErr);
        ASSERT( !lgBoundErr ); /* this should never happen */
        /* deriv is dLambda/dU at Umax, in 1/grain/s */
        deriv = y*c0/(uderiv(Tmax,nd)*Tmax);
        /* estimated FWHM of probability distribution, in Ryd */
        fwhm = sqrt(8.*LN_TWO*c1/deriv);

        NumEvents = POW2(fwhm)*c0/(4.*LN_TWO*c2);
        FwhmRatio = fwhm/Umax;

        /* >>chng 01 nov 15, change ( NumEvents > MAX_EVENTS2 ) --> ( FwhmRatio < FWHM_RATIO2 ), PvH */
        lgDelta = ( FwhmRatio < FWHM_RATIO2 );
        /* high intensity case is always OK since we will use equilibrium treatment */
        lgOK = lgDelta;

        ErrorStart = QH_OK;

        if( lgDelta ) 
        {
                /* in this case we ignore negative rates, equilibrium treatment is good enough */
                lgNegRate = false;
                ErrorStart = MAX2(ErrorStart,QH_DELTA);
        }

        if( lgNegRate )
                ErrorStart = MAX2(ErrorStart,QH_NEGRATE_FAIL);

        ErrorCode = ErrorStart;

        if( trace.lgTrace && trace.lgDustBug )
        {
                double Rate2 = 0.;
                for( int nz=0; nz < gv.bin[nd]->nChrg; nz++ )
                        Rate2 += gv.bin[nd]->chrg[nz]->FracPop*gv.bin[nd]->chrg[nz]->HeatingRate2;

                fprintf( ioQQQ, "   grain heating: %.4e, integral %.4e, total rate %.4e lgNegRate %c\n",
                         gv.bin[nd]->GrainHeat,integral,Phi[0],TorF(lgNegRate));
                fprintf( ioQQQ, "   av grain temp %.4e av grain enthalpy (Ryd) %.4e\n",
                         gv.bin[nd]->tedust,Umax);
                fprintf( ioQQQ, "   fwhm^2/(4ln2*c2/c0): %.4e fwhm (Ryd) %.4e fwhm/Umax %.4e\n",
                         NumEvents,fwhm,FwhmRatio );
                fprintf( ioQQQ, "   HeatingRate1 %.4e HeatingRate2 %.4e lgQHTooWide %c\n",
                         gv.bin[nd]->HeatingRate1*gv.bin[nd]->cnv_H_pCM3, Rate2*gv.bin[nd]->cnv_H_pCM3,
                         TorF(gv.bin[nd]->lgQHTooWide) );
        }

        /* these two variables will bracket qtmin, they should only be needed during the initial search phase */
        minBracket = GRAIN_TMIN;
        maxBracket = gv.bin[nd]->tedust;

        /* >>chng 02 jan 30, introduced lgTried to avoid running GetProbDistr_HighLimit over and over..., PvH */
        lgTried = false;
        /* >>chng 02 aug 06, introduced QH_WIDE_FAIL and nWideFail, PvH */
        nWideFail = 0;
        /* >>chng 03 jan 27, introduced DefFac to increase factor for repeated LOW_FAIL's, PvH */
        DefFac = DEF_FAC;
        /* >>chng 04 nov 10, introduced rel_tol to increase precision in case of repeated CONV_FAIL's, PvH */
        rel_tol = 1.;

        /* if average number of multiple photon events is too high, lgOK is set to true */
        /* >>chng 02 aug 12, added gv.bin[nd]->lgQHTooWide to prevent unnecessary looping here.
         * In general the number of integration steps needed to integrate the probability distribution
         * will increase monotonically with depth into the cloud. Hence, once the distribution becomes
         * too wide to fit into NQGRID steps (which only happens for extremely cold grains in deeply
         * shielded conditions) there is no hope of ever converging GetProbDistr_LowLimit and the code
         * will waste a lot of CPU time establishing this for every zone again. So once the distribution
         * becomes too wide we immediately skip to the analytic approximation to save time, PvH */
        for( i=0; i < LOOP_MAX && !lgOK && !gv.bin[nd]->lgQHTooWide; i++ )
        {
                if( gv.bin[nd]->qtmin >= gv.bin[nd]->tedust )
                {
                        /* >>chng 02 jul 31, was gv.bin[nd]->qtmin = 0.7*gv.bin[nd]->tedust */
                        /* >>chng 03 nov 10, changed Umax/exp(+... to Umax*exp(-... to avoid overflow, PvH */
                        double Ulo = Umax*exp(-sqrt(-log(PROB_CUTOFF_LO)/(4.*LN_TWO))*fwhm/Umax);
                        double MinEnth = exp(gv.bin[nd]->DustEnth[0]);
                        Ulo = MAX2(Ulo,MinEnth);
                        gv.bin[nd]->qtmin = inv_ufunct(Ulo,nd,&lgBoundErr);
                        ASSERT( !lgBoundErr ); /* this should never happen */
                        /* >>chng 02 jul 30, added this test; prevents problems with ASSERT below, PvH */
                        if( gv.bin[nd]->qtmin <= minBracket || gv.bin[nd]->qtmin >= maxBracket )
                                gv.bin[nd]->qtmin = sqrt(minBracket*maxBracket);
                }
                gv.bin[nd]->qtmin = MAX2(gv.bin[nd]->qtmin,GRAIN_TMIN);

                ASSERT( minBracket <= gv.bin[nd]->qtmin && gv.bin[nd]->qtmin <= maxBracket );

                ErrorCode = ErrorStart;

                /* >>chng 01 nov 15, add ( FwhmRatio >= FWHM_RATIO ), PvH */
                if( FwhmRatio >= FWHM_RATIO && NumEvents <= MAX_EVENTS )
                {
                        GetProbDistr_LowLimit(nd,rel_tol,Umax,fwhm,Phi,PhiDrv,qtemp,qprob,dPdlnT,qnbin,
                                              &new_tmin,&nWideFail,&ErrorCode);

                        /* >>chng 02 jan 07, various changes to improve convergence for very cold grains, PvH */
                        if( ErrorCode == QH_DELTA_FAIL && fwhm < Umax && !lgTried )
                        {
                                double dummy;

                                /* this situation can mean two things: either the photon rate is so high that
                                 * the code needs too many steps to integrate the probability distribution,
                                 * or alternatively, tmin is far too low and the code needs too many steps
                                 * to overcome the rising side of the probability distribution.
                                 * So we call GetProbDistr_HighLimit first to determine if the former is the
                                 * case; if that fails then the latter must be true and we reset QH_DELTA_FAIL */
                                ErrorCode = MAX2(ErrorStart,QH_ANALYTIC);
                                /* use dummy to avoid losing estimate for new_tmin from GetProbDistr_LowLimit */
                                /* >>chng 02 aug 06, introduced STRICT and RELAX, PvH */
                                GetProbDistr_HighLimit(nd,STRICT,Umax,fwhm,qtemp,qprob,dPdlnT,&tol,qnbin,&dummy,
                                                       &ErrorCode);

                                if( ErrorCode >= QH_RETRY )
                                {
                                        ErrorCode = QH_DELTA_FAIL;
                                        lgTried = true;
                                }
                        }

                        /* >>chng 02 aug 07 major rewrite of the logic below */
                        if( ErrorCode < QH_NO_REBIN )
                        {
                                if( new_tmin < minBracket || new_tmin > maxBracket )
                                        ++nWideFail;

                                if( nWideFail < WIDE_FAIL_MAX )
                                {
                                        if( new_tmin <= minBracket )
                                                new_tmin = sqrt(gv.bin[nd]->qtmin*minBracket);
                                        if( new_tmin >= maxBracket )
                                                new_tmin = sqrt(gv.bin[nd]->qtmin*maxBracket);
                                }
                                else
                                {
                                        ErrorCode = MAX2(ErrorCode,QH_WIDE_FAIL);
                                }

                                if( ErrorCode == QH_CONV_FAIL )
                                {
                                        rel_tol *= 0.9;
                                }
                        }
                        else if( ErrorCode == QH_LOW_FAIL )
                        {
                                double help1 = gv.bin[nd]->qtmin*sqrt(DefFac);
                                double help2 = sqrt(gv.bin[nd]->qtmin*maxBracket);
                                minBracket = gv.bin[nd]->qtmin;
                                new_tmin = MIN2(help1,help2);
                                /* increase factor in case we get repeated LOW_FAIL's */
                                DefFac += 1.5;
                        }
                        else if( ErrorCode == QH_HIGH_FAIL )
                        {
                                double help = sqrt(gv.bin[nd]->qtmin*minBracket);
                                maxBracket = gv.bin[nd]->qtmin;
                                new_tmin = MAX2(gv.bin[nd]->qtmin/DEF_FAC,help);
                        }
                        else
                        {
                                new_tmin = sqrt(minBracket*maxBracket);
                        }
                }
                else
                {
                        GetProbDistr_HighLimit(nd,STRICT,Umax,fwhm,qtemp,qprob,dPdlnT,&tol,qnbin,&new_tmin,
                                               &ErrorCode);
                }

                gv.bin[nd]->qtmin = new_tmin;

                lgOK = ( ErrorCode < QH_RETRY );

                if( ErrorCode >= QH_FATAL )
                        break;

                if( ErrorCode != QH_LOW_FAIL )
                        DefFac = DEF_FAC;

                if( trace.lgTrace && trace.lgDustBug ) 
                {
                        fprintf( ioQQQ, "   GetProbDistr returns code %d\n", ErrorCode );
                        if( !lgOK )
                        {
                                fprintf( ioQQQ, " >>>>qheat trying another iteration, qtmin bracket %.4e %.4e",
                                         minBracket,maxBracket );
                                fprintf( ioQQQ, " nWideFail %ld\n", nWideFail );
                        }
                }
        }

        if( ErrorCode == QH_WIDE_FAIL )
                gv.bin[nd]->lgQHTooWide = true;

        /* >>chng 03 jan 17, added test for !lgDelta, PvH */
        /* if( gv.bin[nd]->lgQHTooWide ) */
        if( gv.bin[nd]->lgQHTooWide && !lgDelta )
                ErrorCode = MAX2(ErrorCode,QH_WIDE_FAIL);

/*      if( ErrorCode >= QH_RETRY ) */
/*              printf( "      *** PROBLEM  loop not converged, errorcode %d\n",ErrorCode ); */

        /* The quantum heating code tends to run into trouble when it goes deep into the neutral zone,
         * especially if the original spectrum was very hard, as is the case in high excitation PNe or AGN.
         * You then get a bipartition in the spectrum where most of the photons have low energy, while
         * there still are hard X-ray photons left. The fact that the average energy per photon is low
         * forces the quantum code to take tiny little steps when integrating the probability distribution,
         * while the fact that X-ray photons are still present implies that big temperature spikes still
         * occur and hence the temperature distribution is very wide. Therefore the code needs a zillion
         * steps to integrate the probability distribution and simply runs out of room. As a last resort
         * try the analytic approximation with relaxed constraints used below. */
        /* >>chng 02 oct 03, vary Umax and fwhm to force fit with fwhm/Umax remaining constant */
        /* >>chng 03 jan 17, changed test so that last resort always gets tried when lgOK = lgDelta = false, PvH */
        /* if( !lgOK && FwhmRatio >= FWHM_RATIO && NumEvents <= MAX_EVENTS ) */
        if( !lgOK && !lgDelta )
        {
                double Umax2 = Umax*sqrt(tol);
                double fwhm2 = fwhm*sqrt(tol);

                for( i=0; i < LOOP_MAX; ++i )
                {
                        double dummy;

                        ErrorCode2 = MAX2(ErrorStart,QH_ANALYTIC);
                        GetProbDistr_HighLimit(nd,RELAX,Umax2,fwhm2,qtemp,qprob,dPdlnT,&tol,qnbin,&dummy,
                                               &ErrorCode2);

                        lgOK = ( ErrorCode2 < QH_RETRY );
                        if( lgOK )
                        {
                                gv.bin[nd]->qtmin = dummy;
                                ErrorCode = ErrorCode2;
                                break;
                        }
                        else
                        {
                                Umax2 *= sqrt(tol);
                                fwhm2 *= sqrt(tol);
                        }
                }
        }

        if( nzone == 1 )
                gv.bin[nd]->qtmin_zone1 = gv.bin[nd]->qtmin;

        gv.bin[nd]->lgUseQHeat = ( lgOK && !lgDelta );
        gv.bin[nd]->lgEverQHeat = ( gv.bin[nd]->lgEverQHeat || gv.bin[nd]->lgUseQHeat );

        if( lgOK )
        {
                if( trace.lgTrace && trace.lgDustBug )
                        fprintf( ioQQQ, " >>>>qheat converged with code: %d\n", ErrorCode );
        }
        else
        {
                *qnbin = 0;
                ++gv.bin[nd]->QHeatFailures;
                fprintf( ioQQQ, " PROBLEM  qheat did not converge grain %s in zone %ld, error code = %d\n",
                         gv.bin[nd]->chDstLab,nzone,ErrorCode );                
        }

        if( gv.QHPunchFile != NULL && ( iterations.lgLastIt || !gv.lgQHPunLast ) ) 
        {
                fprintf( gv.QHPunchFile, "\nDust Temperature Distribution: grain %s zone %ld\n",
                         gv.bin[nd]->chDstLab,nzone );

                fprintf( gv.QHPunchFile, "Equilibrium temperature: %.2f\n", gv.bin[nd]->tedust );

                if( gv.bin[nd]->lgUseQHeat ) 
                {
                        /* >>chng 01 oct 09, remove qprob from output, it depends on step size, PvH */
                        fprintf( gv.QHPunchFile, "Number of bins: %ld\n", *qnbin );
                        fprintf( gv.QHPunchFile, "  Tgrain      dP/dlnT\n" );
                        for( i=0; i < *qnbin; i++ ) 
                        {
                                fprintf( gv.QHPunchFile, "%.4e %.4e\n", qtemp[i],dPdlnT[i] );
                        }
                }
                else 
                {
                        fprintf( gv.QHPunchFile, "**** quantum heating was not used\n" );
                }
        }

        free ( phiTilde );
        free ( Phi );
        free ( PhiDrv );
        free ( dPdlnT );
        return;
}


/* initialize phiTilde */
STATIC void qheat_init(long nd,
                       /*@out@*/ double phiTilde[],  /* phiTilde[rfield.nupper] */
                       /*@out@*/ double *check)
{
        long i,
          nz;
        double sum = 0.;

        /*@-redef@*/
        enum {DEBUG_LOC=false};
        /*@+redef@*/

        DEBUG_ENTRY( "qheat_init()" );

        /* sanity checks */
        ASSERT( gv.bin[nd]->lgQHeat );
        ASSERT( nd >= 0 && nd < gv.nBin );

        *check = 0.;

        /* >>chng 01 nov 29, rfield.nflux -> gv.qnflux, PvH */
        /* >>chng 03 jan 26, gv.qnflux -> gv.bin[nd]->qnflux, PvH */
        for( i=0; i < gv.bin[nd]->qnflux; i++ )
        {
                phiTilde[i] = 0.;
        }

        /* fill in auxiliary array for quantum heating routine
         * it reshuffles the input spectrum times the cross section to take
         * the photo-electric effect into account. this prevents the quantum
         * heating routine from having to calculate this effect over and over
         * again; it can do a straight integration instead, making the code
         * a lot simpler and faster. this initializes the array for non-ionizing
         * energies, the reshuffling for higher energies is done in the next loop
         * phiTilde has units events/H/s/cell at default depletion */

        double NegHeatingRate = 0.;

        for( nz=0; nz < gv.bin[nd]->nChrg; nz++ )
        {
                double check1 = 0.;
                ChargeBin *gptr = gv.bin[nd]->chrg[nz];

                /* integrate over incident continuum for non-ionizing energies */
                for( i=0; i < MIN2(gptr->ipThresInf,rfield.nflux); i++ )
                {
                        check1 += rfield.SummedCon[i]*gv.bin[nd]->dstab1[i]*rfield.anu[i];
                        phiTilde[i] += gptr->FracPop*rfield.SummedCon[i]*gv.bin[nd]->dstab1[i];
                }

                /* >>chng 01 mar 02, use new expresssions for grain cooling and absorption
                 * cross sections following the discussion with Joe Weingartner, PvH */
                for( i=gptr->ipThresInf; i < rfield.nflux; i++ )
                {
                        long ipLo2 = gptr->ipThresInfVal;
                        double cs1 = ( i >= ipLo2 ) ? gv.bin[nd]->dstab1[i]*gptr->yhat_primary[i] : 0.;

                        check1 += rfield.SummedCon[i]*gptr->fac1[i];
                        /* this accounts for the photons that are fully absorbed by grain */
                        phiTilde[i] += gptr->FracPop*rfield.SummedCon[i]*MAX2(gv.bin[nd]->dstab1[i]-cs1,0.);

                        /* >>chng 01 oct 10, use bisection search to find ip. On C scale now */

                        /* this accounts for photons that eject an electron from the valence band */
                        if( cs1 > 0. )
                        {
                                /* we treat photo-ejection and all subsequent de-excitation cascades
                                 * from the conduction/valence band as one simultaneous event */
                                /* the condition cs1 > 0. assures i >= ipLo2 */
                                /* ratio is number of ejected electrons per primary ionization */
                                double ratio = ( gv.lgWD01 ) ? 1. : gptr->yhat[i]/gptr->yhat_primary[i];
                                /* ehat is average energy of ejected electron at infinity */
                                double ehat = gptr->ehat[i];
                                double cool1, sign = 1.;
                                realnum xx;

                                if( gptr->DustZ <= -1 )
                                        cool1 = gptr->ThresSurf + gptr->PotSurf + ehat;
                                else
                                        cool1 = gptr->ThresSurfVal + gptr->PotSurf + ehat;
                                /* secondary electrons are assumed to have the same Elo and Ehi as the
                                 * primary electrons that excite them. This neglects the threshold for
                                 * the ejection of the secondary electron and can cause xx to become
                                 * negative if Ehi is less than that threshold. To conserve energy we
                                 * will simply assume a negative rate here. Since secondary electrons
                                 * are generally not important this should have little impact on the
                                 * overall temperature distribution */
                                xx = rfield.anu[i] - (realnum)(ratio*cool1);
                                if( xx < 0.f )
                                {
                                        xx = -xx;
                                        sign = -1.;
                                }
                                long ipLo = hunt_bisect( gv.anumin, i+1, xx );
                                /* for grains in hard X-ray environments, the coarseness of the grid can
                                 * lead to inaccuracies in the integral over phiTilde that would trip the
                                 * sanity check in qheat(), here we correct for the energy mismatch */
                                double corr = xx/rfield.anu[ipLo];
                                phiTilde[ipLo] += sign*corr*gptr->FracPop*rfield.SummedCon[i]*cs1;
                        }

                        /* no need to account for photons that eject an electron from the conduction band */
                        /* >>chng 01 dec 11, cool2 always equal to rfield.anu[i] -> no grain heating */
                }

                *check += gptr->FracPop*check1*EN1RYD*gv.bin[nd]->cnv_H_pCM3;

                sum += gptr->FracPop*check1*EN1RYD*gv.bin[nd]->cnv_H_pCM3;

                if( DEBUG_LOC )
                {
                        double integral = 0.;
                        for( i=0; i < gv.bin[nd]->qnflux; i++ )
                        {
                                integral += phiTilde[i]*gv.bin[nd]->cnv_H_pCM3*rfield.anu[i]*EN1RYD;
                        }
                        dprintf( ioQQQ, " integral test 1: integral %.6e %.6e\n", integral, sum );
                }

                /* add quantum heating due to recombination of electrons, subtract thermionic cooling */

                /* gptr->HeatingRate2 is net heating rate in erg/H/s at standard depl
                 * includes contributions for recombining electrons, autoionizing electrons
                 * subtracted by thermionic emissions here since it is inverse process
                 *
                 * NB - in extreme conditions this rate may be negative (if there
                 * is an intense radiation field leading to very hot grains, but no ionizing
                 * photons, hence very few free electrons). we assume that the photon rates
                 * are high enough under those circumstances to avoid phiTilde becoming negative,
                 * but we will check that in qheat1 anyway. */

                /* >>chng 03 nov 06, check for extremely low HeatingRate and save CPU time, pah_crash.in, PvH */
                if( gptr->HeatingRate2*gv.bin[nd]->cnv_H_pCM3 > 0.05*CONSERV_TOL*gv.bin[nd]->GrainHeat ) 
                {
                        double *RateArr,Sum,ESum,DSum,Delta,E_av2,Corr;
                        double fac = BOLTZMANN/EN1RYD*phycon.te;
                        /* E0 is barrier that electron needs to overcome, zero for positive grains */
                        /* >>chng 03 jan 23, added second term to correctly account for autoionizing states
                         *                   where ThresInfInc is negative, tested in small_grain.in, PvH */
                        double E0 = -(MIN2(gptr->PotSurfInc,0.) + MIN2(gptr->ThresInfInc,0.));
                        /* >>chng 01 mar 02, this should be energy gap between top electron and infinity, PvH */
                        /* >>chng 01 nov 21, use correct barrier: ThresInf[nz] -> ThresInfInc[nz], PvH */
                        /* >>chng 03 jan 23, replaced -E0 with MIN2(PotSurfInc[nz],0.), PvH */
                        double Einf = gptr->ThresInfInc + MIN2(gptr->PotSurfInc,0.);
                        /* this is average energy deposited by one event, in erg
                         * this value is derived from distribution assumed here, and may
                         * not be the same as HeatElectrons/(CollisionRateElectr*eta) !! */
                        /* >>chng 01 nov 21, use correct barrier: ThresInf[nz] -> ThresInfInc[nz], PvH */
                        /* >>chng 03 jan 23, replaced ThresInfInc[nz] with MAX2(ThresInfInc[nz],0.), PvH */
                        double E_av = MAX2(gptr->ThresInfInc,0.)*EN1RYD + 2.*BOLTZMANN*phycon.te;
                        /* this is rate in events/H/s at standard depletion */
                        double rate = gptr->HeatingRate2/E_av;

                        double ylo = -exp(-E0/fac);
                        /* this is highest kinetic energy of electron that can be represented in phiTilde */
                        /* >>chng 01 nov 29, rfield.nflux -> gv.qnflux, PvH */
                        /* >>chng 03 jan 26, gv.qnflux -> gv.bin[nd]->qnflux, PvH */
                        double Ehi = gv.anumax[gv.bin[nd]->qnflux-1]-Einf;
                        double yhi = ((E0-Ehi)/fac-1.)*exp(-Ehi/fac);
                        /* renormalize rate so that integral over phiTilde*anu gives correct total energy */
                        rate /= yhi-ylo;

                        /* correct for fractional population of this charge state */
                        rate *= gptr->FracPop;

                        /* >>chng 03 jan 24, add code to correct for discretization errors, hotdust.in, PvH */
                        RateArr=(double*)MALLOC((size_t)((unsigned)gv.bin[nd]->qnflux*sizeof(double)));
                        Sum = ESum = DSum = 0.;

                        /* >>chng 04 jan 21, replaced gv.bin[nd]->qnflux -> gv.bin[nd]->qnflux2, PvH */
                        for( i=0; i < gv.bin[nd]->qnflux2; i++ ) 
                        {
                                Ehi = gv.anumax[i] - Einf;
                                if( Ehi >= E0 ) 
                                {
                                        /* Ehi is kinetic energy of electron at infinity */
                                        yhi = ((E0-Ehi)/fac-1.)*exp(-Ehi/fac);
                                        /* >>chng 01 mar 24, use MAX2 to protect against roundoff error, PvH */
                                        RateArr[i] = rate*MAX2(yhi-ylo,0.);
                                        Sum += RateArr[i];
                                        ESum += rfield.anu[i]*RateArr[i];
#                                       ifndef NDEBUG
                                        DSum += rfield.widflx[i]*RateArr[i];
#                                       endif
                                        ylo = yhi;
                                }
                                else
                                {
                                        RateArr[i] = 0.;
                                }
                        }
                        E_av2 = ESum/Sum*EN1RYD;
                        Delta = DSum/Sum*EN1RYD;
                        ASSERT( fabs(E_av-E_av2) <= Delta );
                        Corr = E_av/E_av2;

                        for( i=0; i < gv.bin[nd]->qnflux2; i++ ) 
                        {
                                phiTilde[i] += RateArr[i]*Corr;
                        }

                        sum += gptr->FracPop*gptr->HeatingRate2*gv.bin[nd]->cnv_H_pCM3;

                        if( DEBUG_LOC )
                        {
                                double integral = 0.;
                                for( i=0; i < gv.bin[nd]->qnflux; i++ )
                                {
                                        integral += phiTilde[i]*gv.bin[nd]->cnv_H_pCM3*rfield.anu[i]*EN1RYD;
                                }
                                dprintf( ioQQQ, " integral test 2: integral %.6e %.6e\n", integral, sum );
                        }

                        free( RateArr );
                }
                else
                {
                        NegHeatingRate += gptr->FracPop*gptr->HeatingRate2*gv.bin[nd]->cnv_H_pCM3;
                }
        }

        /* ============================================================================= */

        /* add quantum heating due to molecule/ion collisions */

        /* gv.bin[nd]->HeatingRate1 is heating rate in erg/H/s at standard depl
         * includes contributions from molecules/neutral atoms and recombining ions
         *
         * in fully ionized conditions electron heating rates will be much higher
         * than ion and molecule rates since electrons are so much faster and grains
         * tend to be positive. in non-ionized conditions the main contribution will
         * come from neutral atoms and molecules, so it is appropriate to treat both
         * the same. in fully ionized conditions we don't care since unimportant.
         *
         * NB - if grains are hotter than ambient gas, the heating rate may become negative.
         * if photon rates are not high enough to prevent phiTilde from becoming negative,
         * we will raise a flag while calculating the quantum heating in qheat1 */

        /* >>chng 03 nov 06, check for extremely low HeatingRate and save CPU time, PvH */
        if( gv.bin[nd]->HeatingRate1*gv.bin[nd]->cnv_H_pCM3 > 0.05*CONSERV_TOL*gv.bin[nd]->GrainHeat )
        {
                /* limits for Taylor expansion of (1+x)*exp(-x) */
                /* these choices will assure only 6 digits precision */
                const double LIM2 = pow(3.e-6,1./3.);
                const double LIM3 = pow(8.e-6,1./4.);
                /* if gas temperature is higher than grain temperature we will
                 * consider Maxwell-Boltzmann distribution of incoming particles
                 * and ignore distribution of outgoing particles, if grains
                 * are hotter than ambient gas, we use reverse treatment */
                double fac = BOLTZMANN/EN1RYD*MAX2(phycon.te,gv.bin[nd]->tedust);
                /* this is average energy deposited/extracted by one event, in erg */
                double E_av = 2.*BOLTZMANN*MAX2(phycon.te,gv.bin[nd]->tedust);
                /* this is rate in events/H/s at standard depletion */
                double rate = gv.bin[nd]->HeatingRate1/E_av;

                double ylo = -1.;
                /* this is highest energy of incoming/outgoing particle that can be represented in phiTilde */
                /* >>chng 01 nov 29, rfield.nflux -> gv.qnflux, PvH */
                /* >>chng 03 jan 26, gv.qnflux -> gv.bin[nd]->qnflux, PvH */
                double Ehi = gv.anumax[gv.bin[nd]->qnflux-1];
                double yhi = -(Ehi/fac+1.)*exp(-Ehi/fac);
                /* renormalize rate so that integral over phiTilde*anu gives correct total energy */
                rate /= yhi-ylo;

                for( i=0; i < gv.bin[nd]->qnflux2; i++ ) 
                {
                        /* Ehi is kinetic energy of incoming/outgoing particle
                         * we assume that Ehi-E0 is deposited/extracted from grain */
                        /* Ehi = gv.anumax[i]; */
                        double x = gv.anumax[i]/fac;
                        /* (1+x)*exp(-x) = 1 - 1/2*x^2 + 1/3*x^3 - 1/8*x^4 + O(x^5)
                         *               = 1 - Sum_n=2^infty (-x)^n/(n*(n-2)!)      */
                        if( x > LIM3 )
                                yhi = -(x+1.)*exp(-x);
                        else if( x > LIM2 )
                                yhi = -(((1./3.)*x - 0.5)*x*x + 1.);
                        else
                                yhi = -(1. - 0.5*x*x);

                        /* >>chng 01 mar 24, use MAX2 to protect against roundoff error, PvH */
                        phiTilde[i] += rate*MAX2(yhi-ylo,0.);
                        ylo = yhi;
                }

                sum += gv.bin[nd]->HeatingRate1*gv.bin[nd]->cnv_H_pCM3;

                if( DEBUG_LOC )
                {
                        double integral = 0.;
                        for( i=0; i < gv.bin[nd]->qnflux; i++ )
                        {
                                integral += phiTilde[i]*gv.bin[nd]->cnv_H_pCM3*rfield.anu[i]*EN1RYD;
                        }
                        dprintf( ioQQQ, " integral test 3: integral %.6e %.6e\n", integral, sum );
                }
        }
        else
        {
                NegHeatingRate += gv.bin[nd]->HeatingRate1*gv.bin[nd]->cnv_H_pCM3;
        }

        /* here we account for the negative heating rates, we simply do that by scaling the entire
         * phiTilde array down by a constant factor such that the total amount of energy is conserved
         * This treatment assures that phiTilde never goes negative, which avoids problems further on */
        if( NegHeatingRate < 0. )
        {
                double scale_fac = (sum+NegHeatingRate)/sum;
                for( i=0; i < gv.bin[nd]->qnflux; i++ )
                        phiTilde[i] *= scale_fac;

                sum += NegHeatingRate;

                if( DEBUG_LOC )
                {
                        double integral = 0.;
                        for( i=0; i < gv.bin[nd]->qnflux; i++ )
                        {
                                integral += phiTilde[i]*gv.bin[nd]->cnv_H_pCM3*rfield.anu[i]*EN1RYD;
                        }
                        dprintf( ioQQQ, " integral test 4: integral %.6e %.6e\n", integral, sum );
                }
        }

        return;
}


/*******************************************************************************************
 *
 * GetProbDistr_LowLimit: main routine for calculating non-equilibrium heating of grains
 *
 * This routine implements the algorithm outlined in:
 * >>refer      grain   physics Guhathakurtha & Draine, 1989, ApJ, 345, 230
 *
 * The original (fortran) version of the code was written by Kevin Volk.
 *
 * Heavily modified and adapted for new style grains by Peter van Hoof.
 *
 *******************************************************************************************/

STATIC void GetProbDistr_LowLimit(long int nd,
                                  double rel_tol,
                                  double Umax,
                                  double fwhm,
                                  /*@in@*/ double Phi[],     /* Phi[NQGRID]      */
                                  /*@in@*/ double PhiDrv[],  /* PhiDrv[NQGRID]   */
                                  /*@out@*/ double qtemp[],  /* qtemp[NQGRID]    */
                                  /*@out@*/ double qprob[],  /* qprob[NQGRID]    */
                                  /*@out@*/ double dPdlnT[], /* dPdlnT[NQGRID]   */
                                  /*@out@*/ long int *qnbin,
                                  /*@out@*/ double *new_tmin,
                                  long *nWideFail,
                                  /*@out@*/ QH_Code *ErrorCode)
{
        bool lgAllNegSlope,
          lgBoundErr;
        long int j,
          k,
          l,
          nbad,
          nbin,
          nend=0,
          nmax,
          nok,
          nstart=0,
          nstart2=0;
        double dCool,
          delu[NQGRID],
          dlnLdlnT,
          dlnpdlnU,
          fac = 0.,
          Lambda[NQGRID],
          maxVal,
          NextStep,
          p[NQGRID],
          qtmin1, 
          RadCooling,
          sum,
          u1[NQGRID],
          y;


        DEBUG_ENTRY( "GetProbDistr_LowLimit()" );

        /* sanity checks */
        ASSERT( nd >= 0 && nd < gv.nBin );

        if( trace.lgTrace && trace.lgDustBug )
        {
                fprintf( ioQQQ, "   GetProbDistr_LowLimit called for grain %s\n", gv.bin[nd]->chDstLab );
                fprintf( ioQQQ, "    got qtmin1 %.4e\n", gv.bin[nd]->qtmin);
        }

        qtmin1 = gv.bin[nd]->qtmin;
        qtemp[0] = qtmin1;
        /* u1 holds enthalpy in Ryd/grain */
        u1[0] = ufunct(qtemp[0],nd,&lgBoundErr);
        ASSERT( !lgBoundErr ); /* this should never happen */
        /* >>chng 00 mar 22, taken out factor 4, factored in hden and dstAbund
         * interpolate in dstems array instead of integrating explicitly, by PvH */
        splint_safe(gv.dsttmp,gv.bin[nd]->dstems,gv.bin[nd]->dstslp2,NDEMS,log(qtemp[0]),&y,&lgBoundErr);
        ASSERT( !lgBoundErr ); /* this should never happen */
        /* Lambda holds the radiated energy for grains in this bin, in Ryd/s/grain */
        Lambda[0] = exp(y)*gv.bin[nd]->cnv_H_pGR/EN1RYD;
        /* set up first step of integration */
        /* >>chng 01 nov 14, set to 2.*Lambda[0]/Phi[0] instead of u1[0],
         * this choice assures that p[1] doesn't make a large jump from p[0], PvH */
        delu[0] = 2.*Lambda[0]/Phi[0];
        p[0] = PROB_CUTOFF_LO;
        dPdlnT[0] = p[0]*qtemp[0]*uderiv(qtemp[0],nd);
        RadCooling = 0.5*p[0]*Lambda[0]*delu[0];
        NextStep = 0.01*Lambda[0]/Phi[0];
        /* >>chng 03 nov 10, added extra safeguard against stepsize too small, PvH */
        if( NextStep < 0.05*DBL_EPSILON*u1[0] )
        {
                *ErrorCode = MAX2(*ErrorCode,QH_STEP_FAIL);
                return;
        }
        else if( NextStep < 5.*DBL_EPSILON*u1[0] )
        {
                /* try a last resort... */
                NextStep *= 100.;
        }

        nbad = 0;
        k = 0;

        *qnbin = 0;
        *new_tmin = qtmin1;
        lgAllNegSlope = true;
        maxVal = dPdlnT[0];
        nmax = 0;

        /* this test neglects a negative contribution which is impossible to calculate, so it may
         * fail to detect cases where the probability distribution starts dropping immediately,
         * we will use a second test using the variable lgAllNegSlope below to catch those cases, PvH */
        spldrv_safe(gv.dsttmp,gv.bin[nd]->dstems,gv.bin[nd]->dstslp2,NDEMS,log(qtemp[0]),&dlnLdlnT,&lgBoundErr);
        ASSERT( !lgBoundErr ); /* this should never happen */
        dlnpdlnU = u1[0]*Phi[0]/Lambda[0] - dlnLdlnT*u1[0]/(qtemp[0]*uderiv(qtemp[0],nd));
        if( dlnpdlnU < 0. )
        {
                /* >>chng 03 nov 06, confirm this by integrating first step..., pah_crash.in, PvH */
                (void)TryDoubleStep(u1,delu,p,qtemp,Lambda,Phi,PhiDrv,NextStep,&dCool,k,nd,&lgBoundErr);
                dPdlnT[2] = p[2]*qtemp[2]*uderiv(qtemp[2],nd);

                if( dPdlnT[2] < dPdlnT[0] )
                {
                        /* if dPdlnT starts falling immediately, 
                         * qtmin1 was too high and convergence is impossible */
                        *ErrorCode = MAX2(*ErrorCode,QH_HIGH_FAIL);
                        return;
                }
        }

        /* NB NB -- every break in this loop should set *ErrorCode (except for regular stop criterion) !! */
        for( l=0; l < MAX_LOOP; ++l )
        {
                double RelError = TryDoubleStep(u1,delu,p,qtemp,Lambda,Phi,PhiDrv,NextStep,&dCool,k,nd,&lgBoundErr);

                /* this happens if the grain temperature in qtemp becomes higher than GRAIN_TMAX
                 * nothing that TryDoubleStep returns can be trusted, so this check should be first */
                if( lgBoundErr )
                {
                        nbad += 2;
                        *ErrorCode = MAX2(*ErrorCode,QH_THIGH_FAIL);
                        break;
                }

                /* estimate new stepsize */
                if( RelError > rel_tol*QHEAT_TOL )
                {
                        nbad += 2;

                        /* step is rejected, decrease stepsize and try again */
                        NextStep *= sqrt(0.9*rel_tol*QHEAT_TOL/RelError);

                        /* stepsize too small, this can happen at extreme low temperatures */
                        if( NextStep < 5.*DBL_EPSILON*u1[k] )
                        {
                                *ErrorCode = MAX2(*ErrorCode,QH_STEP_FAIL);
                                break;
                        }

                        continue;
                }
                else
                {
                        /* step was OK, adjust stepsize */
                        k += 2;

                        /* >>chng 03 nov 10, safeguard against division by zero, PvH */
                        NextStep *= MIN2(pow(0.9*rel_tol*QHEAT_TOL/MAX2(RelError,1.e-50),1./3.),4.);
                        NextStep = MIN2(NextStep,Lambda[k]/Phi[0]);
                }

                dPdlnT[k-1] = p[k-1]*qtemp[k-1]*uderiv(qtemp[k-1],nd);
                dPdlnT[k] = p[k]*qtemp[k]*uderiv(qtemp[k],nd);

                lgAllNegSlope = lgAllNegSlope && ( dPdlnT[k] < dPdlnT[k-2] );

                if( dPdlnT[k-1] > maxVal )
                {
                        maxVal = dPdlnT[k-1];
                        nmax = k-1;
                }
                if( dPdlnT[k] > maxVal )
                {
                        maxVal = dPdlnT[k];
                        nmax = k;
                }

                RadCooling += dCool;

//              if( nzone >= 24 && nd == 0 ) {
//              printf(" k %ld T[k] %.6e U[k] %.6e p[k] %.6e dPdlnT[k] %.6e\n",k-1,qtemp[k-1],u1[k-1],p[k-1],dPdlnT[k-1]);
//              printf(" k %ld T[k] %.6e U[k] %.6e p[k] %.6e dPdlnT[k] %.6e\n",k,qtemp[k],u1[k],p[k],dPdlnT[k]);
//              }

                /* if qtmin is far too low, p[k] can become extremely large, exceeding
                 * even double precision range. the following check should prevent overflows */
                /* >>chng 01 nov 07, sqrt(DBL_MAX) -> sqrt(DBL_MAX/100.) so that sqrt(p[k]*p[k+1]) is safe */
                if( p[k] > sqrt(DBL_MAX/100.) ) 
                {
                        *ErrorCode = MAX2(*ErrorCode,QH_LOW_FAIL);
                        break;

#if 0
                        /* >>chng 01 apr 21, change DBL_MAX -> DBL_MAX/100. to work around
                         * a bug in the Compaq C compiler V6.3-025 when invoked with -fast, PvH */
                        for( j=0; j <= k; j++ ) 
                        {
                                p[j] /= DBL_MAX/100.;
                                dPdlnT[j] /= DBL_MAX/100.;
                        }
                        RadCooling /= DBL_MAX/100.;
#endif
                }

                /* this may catch a bug in the Compaq C compiler V6.3-025
                 * if this gets triggered, try compiling with -ieee */
                ASSERT( p[k] > 0. && dPdlnT[k] > 0. && RadCooling > 0. );

                /* do a check for negative slope and if there will be enough room to store results */
                if( k > 0 && k%NQTEST == 0 )
                {
                        double wid, avStep, factor;
                        /* >>chng 02 jul 31, do additional test for HIGH_FAIL,
                         * first test before main loop doesn't catch everything, PvH */
                        if( lgAllNegSlope )
                        {
                                *ErrorCode = MAX2(*ErrorCode,QH_HIGH_FAIL);
                                break;
                        }

                        /* this is a lower limit for the total width of the probability distr */
                        /* >>chng 02 jan 30, corrected calculation of wid and avStep, PvH */
                        wid = (sqrt(-log(PROB_CUTOFF_LO)/(4.*LN_TWO)) +
                               sqrt(-log(PROB_CUTOFF_HI)/(4.*LN_TWO)))*fwhm/Umax;
                        avStep = log(u1[k]/u1[0])/(double)k;
                        /* make an estimate for the number of steps needed */
                        /* >>chng 02 jan 30, included factor 1.5 because stepsize increases near peak, PvH */
                        /* >>chng 02 aug 06, changed 1.5 to sliding scale because of laqheat2.in test, PvH */
                        factor = 1.1 + 3.9*(1.0 - sqrt((double)k/(double)NQGRID));
                        if( wid/avStep > factor*(double)NQGRID )
                        {
                                *ErrorCode = MAX2(*ErrorCode,QH_ARRAY_FAIL);
                                break;
                        }
                }

                /* if we run out of room to store results, do regular break
                 * the code below will sort out if integration is valid or not */
                if( k >= NQGRID-2 )
                {
                        *ErrorCode = MAX2(*ErrorCode,QH_ARRAY_FAIL);
                        break;
                }

                /* force thermal equilibrium of the grains */
                fac = RadCooling*gv.bin[nd]->cnv_GR_pCM3*EN1RYD/gv.bin[nd]->GrainHeat;

                /* this is regular stop criterion */
                if( dPdlnT[k] < dPdlnT[k-1] && dPdlnT[k]/fac < PROB_CUTOFF_HI )
                {
                        break;
                }
        }

        if( l == MAX_LOOP )
                *ErrorCode = MAX2(*ErrorCode,QH_LOOP_FAIL);

        nok = k;
        nbin = k+1;

        /* there are insufficient bins to attempt rebinning */
        if( *ErrorCode < QH_NO_REBIN && nbin < NQMIN ) 
                *ErrorCode = MAX2(*ErrorCode,QH_NBIN_FAIL);

        /* >>chng 02 aug 07, do some basic checks on the distribution first */
        if( *ErrorCode < QH_NO_REBIN )
                ScanProbDistr(u1,dPdlnT,nbin,maxVal,nmax,qtmin1,&nstart,&nstart2,&nend,nWideFail,ErrorCode);

        if( *ErrorCode >= QH_NO_REBIN )
        {
                return;
        }

        for( j=0; j < nbin; j++ )
        {
                p[j] /= fac;
                dPdlnT[j] /= fac;
        }
        RadCooling /= fac;

        /* >>chng 02 aug 08, moved RebinQHeatResults from here further down, this improves new_tmin estimate */
        *new_tmin = 0.;
        for( j=nstart; j < nbin; j++ ) 
        {
                if( dPdlnT[j] < PROB_CUTOFF_LO ) 
                {
                        *new_tmin = qtemp[j];
                }
                else 
                {
                        if( j == nstart )
                        {
                                /* if dPdlnT[nstart] is too high, but qtmin1 is already close to GRAIN_TMIN,
                                 * then don't bother signaling a QH_BOUND_FAIL. grains below GRAIN_TMIN have the
                                 * peak of their thermal emission beyond 3 meter, so they really are irrelevant
                                 * since free-free emission from electrons will drown this grain emission... */
                                if( dPdlnT[j] > SAFETY*PROB_CUTOFF_LO && qtmin1 > 1.2*GRAIN_TMIN )
                                        *ErrorCode = MAX2(*ErrorCode,QH_BOUND_FAIL);

                                /* >>chng 02 aug 11, use nstart2 for more reliable extrapolation */
                                if( dPdlnT[nstart2] < 0.999*dPdlnT[nstart2+NSTARTUP] ) 
                                {
                                        /* >>chng 02 aug 09, new formula for extrapolating new_tmin, PvH */
                                        /* this assumes that at low temperatures the behaviour
                                         * is as follows:   dPdlnT(T) = C1 * exp( -C2/T**3 ) */
                                        double T1 = qtemp[nstart2];
                                        double T2 = qtemp[nstart2+NSTARTUP];
                                        double delta_y = log(dPdlnT[nstart2+NSTARTUP]/dPdlnT[nstart2]);
                                        double c2 = delta_y/(1./POW3(T1)-1./POW3(T2));
                                        double help = c2/POW3(T1) + log(dPdlnT[nstart2]/PROB_CUTOFF_LO);
                                        *new_tmin = pow(c2/help,1./3.);
                                }

                                /* >>chng 04 nov 09, in case of lower bound failure, assure qtmin is lowered, PvH */ 
                                if( dPdlnT[j] > SAFETY*PROB_CUTOFF_LO && *new_tmin >= qtmin1 )
                                {
                                        double delta_x = log(qtemp[nstart2+NSTARTUP]/qtemp[nstart2]);
                                        double delta_y = log(dPdlnT[nstart2+NSTARTUP]/dPdlnT[nstart2]);
                                        delta_x *= log(PROB_CUTOFF_LO/dPdlnT[nstart2])/delta_y;
                                        *new_tmin = qtemp[nstart2]*exp(delta_x);
                                        if( *new_tmin < qtmin1 )
                                                /* in general this estimate will be too low -> use geometric mean */
                                                *new_tmin = sqrt( *new_tmin*qtmin1 );
                                        else
                                                /* last resort... */
                                                *new_tmin = qtmin1/DEF_FAC;
                                }
                        }
                        break;
                }
        }
        *new_tmin = MAX3(*new_tmin,qtmin1/DEF_FAC,GRAIN_TMIN);

        ASSERT( *new_tmin < gv.bin[nd]->tedust );

        /* >>chng 02 jan 30, prevent excessive looping when prob distribution simply won't fit, PvH */
        if( dPdlnT[nbin-1] > SAFETY*PROB_CUTOFF_HI )
        {
                if( *ErrorCode == QH_ARRAY_FAIL || *ErrorCode == QH_LOOP_FAIL )
                {
                        ++(*nWideFail);

                        if( *nWideFail < WIDE_FAIL_MAX )
                        {
                                /* this indicates that low end was OK, but we ran out of room
                                 * to store the high end -> try GetProbDistr_HighLimit instead */
                                *ErrorCode = MAX2(*ErrorCode,QH_DELTA_FAIL);
                        }
                        else
                        {
                                *ErrorCode = MAX2(*ErrorCode,QH_WIDE_FAIL);
                        }
                }
                else
                {
                        *ErrorCode = MAX2(*ErrorCode,QH_BOUND_FAIL);
                }
        }

        /* >>chng 01 may 11, rebin the quantum heating results
         *
         * for grains in intense radiation fields, the code needs high resolution for stability
         * and therefore produces lots of small bins, even though the grains never make large
         * excurions from the equilibrium temperature; adding in the resulting spectra in RT_diffuse
         * takes up an excessive amount of CPU time where most CPU is spent on grains for which
         * the quantum treatment matters least, and moreover on temperature bins with very low
         * probability; rebinning the results on a coarser grid should help reduce the overhead */
        /* >>chng 02 aug 07, use nstart and nend while rebinning */

        nbin = RebinQHeatResults(nd,nstart,nend,p,qtemp,qprob,dPdlnT,u1,delu,Lambda,ErrorCode);

        /* >>chng 01 jul 13, add fail-safe for failure in RebinQHeatResults */
        if( nbin == 0 )
        {
                return;
        }

        *qnbin = nbin;

        sum = 0.;
        for( j=0; j < nbin; j++ )
        {
                sum += qprob[j];
        }

        /* the fact that the probability normalization fails may indicate that the distribution is
         * too close to a delta function to resolve, but another possibility is that the radiation
         * field is extremely diluted allowing a sizable fraction of the grains to cool below
         * GRAIN_TMIN. In the latter case we don't raise QH_CONV_FAIL since these very cool grains
         * only contribute at very long radio wavelengths (more than 1 meter) */
        if( fabs(sum-1.) > PROB_TOL && qtmin1 > 1.2*GRAIN_TMIN )
                *ErrorCode = MAX2(*ErrorCode,QH_CONV_FAIL);

        if( trace.lgTrace && trace.lgDustBug )
        {
                fprintf( ioQQQ,
                         "    zone %ld %s nbin %ld nok %ld nbad %ld total prob %.4e rel_tol %.3e new_tmin %.4e\n",
                         nzone,gv.bin[nd]->chDstLab,nbin,nok,nbad,sum,rel_tol,*new_tmin );
        }
        return;
}


/* try two consecutive integration steps using stepsize "step/2." (yielding p[k]),
 * and also one double integration step using stepsize "step" (yielding p2k).
 * the difference fabs(p2k-p[k])/(3.*p[k]) can be used to estimate the relative
 * accuracy of p[k] and will be used to adapt the stepsize to an optimal value */
STATIC double TryDoubleStep(double u1[],
                            double delu[],
                            double p[],
                            double qtemp[],
                            double Lambda[],
                            double Phi[],
                            double PhiDrv[],
                            double step,
                            /*@out@*/ double *cooling,
                            long index,
                            long nd,
                            /*@out@*/ bool *lgBoundFail)
{
        long i,
          j,
          jlo,
          k=-1000;
        double bval_jk,
          cooling2,
          p2k,
          p_max,
          RelErrCool,
          RelErrPk,
          sum,
          sum2 = -DBL_MAX,
          trap1,
          trap12 = -DBL_MAX,
          trap2,
          uhi,
          ulo,
          umin,
          y;

        DEBUG_ENTRY( "TryDoubleStep()" );

        /* sanity checks */
        ASSERT( index >= 0 && index < NQGRID-2 && nd >= 0 && nd < gv.nBin && step > 0. );

        ulo = rfield.anu[0];
        /* >>chng 01 nov 29, rfield.nflux -> gv.qnflux, PvH */
        /* >>chng 03 jan 26, gv.qnflux -> gv.bin[nd]->qnflux, PvH */
        uhi = rfield.anu[gv.bin[nd]->qnflux-1];

        /* >>chng 01 nov 21, skip initial bins if they have very low probability */
        p_max = 0.;
        for( i=0; i <= index; i++ )
                p_max = MAX2(p_max,p[i]);
        jlo = 0;
        while( p[jlo] < PROB_CUTOFF_LO*p_max )
                jlo++;

        for( i=1; i <= 2; i++ )
        {
                bool lgErr;
                long ipLo = 0;
                long ipHi = gv.bin[nd]->qnflux-1;
                k = index + i;
                delu[k] = step/2.;
                u1[k] = u1[k-1] + delu[k];
                qtemp[k] = inv_ufunct(u1[k],nd,lgBoundFail);
                splint_safe(gv.dsttmp,gv.bin[nd]->dstems,gv.bin[nd]->dstslp2,NDEMS,log(qtemp[k]),&y,&lgErr);
                *lgBoundFail = *lgBoundFail || lgErr;
                Lambda[k] = exp(y)*gv.bin[nd]->cnv_H_pGR/EN1RYD;

                sum = sum2 = 0.;
                trap1 = trap2 = trap12 = 0.;

                /* this loop uses up a large fraction of the total CPU time, it should be well optimized */
                for( j=jlo; j < k; j++ )
                {
                        umin = u1[k] - u1[j];

                        if( umin >= uhi ) 
                        {
                                /* for increasing j, umin will decrease monotonically. If ( umin > uhi ) holds for
                                 * the current value of j, it must have held for the previous value as well. Hence
                                 * both trap1 and trap2 are zero at this point and we would only be adding zero
                                 * to sum. Therefore we skip this step to save CPU time */
                                continue;
                        }
                        else if( umin > ulo )
                        {
                                /* do a bisection search such that rfield.anu[ipLo] <= umin < rfield.anu[ipHi]
                                 * ipoint doesn't always give the correct index into anu (it works for AnuOrg)
                                 * bisection search is also faster, which is important here to save CPU time.
                                 * on the first iteration ipLo equals 0 and the first while loop will be skipped;
                                 * after that umin is monotonically decreasing, and ipHi is retained from the
                                 * previous iteration since it is a valid upper limit; ipLo will equal ipHi-1 */
                                long ipStep = 1;
                                /* >>chng 03 feb 03 rjrw: hunt for lower bracket */
                                while( rfield.anu[ipLo] > (realnum)umin )
                                {
                                        ipHi = ipLo;
                                        ipLo -= ipStep;
                                        if( ipLo <= 0 ) 
                                        {
                                                ipLo = 0;
                                                break;
                                        }
                                        ipStep *= 2;
                                }
                                /* now do regular bisection search */
                                while( ipHi-ipLo > 1 )
                                {
                                        long ipMd = (ipLo+ipHi)/2;
                                        if( rfield.anu[ipMd] > (realnum)umin )
                                                ipHi = ipMd;
                                        else
                                                ipLo = ipMd;
                                }
                                bval_jk = Phi[ipLo] + (umin - rfield.anu[ipLo])*PhiDrv[ipLo];
                        }
                        else
                        {
                                bval_jk = Phi[0];
                        }

                        /* these two quantities are needed to take double step from index -> index+2 */
                        trap12 = trap1;
                        sum2 = sum;

                        /* bval_jk*gv.bin[nd]->cnv_CM3_pGR is the total excitation rate from j to k and
                         * higher due to photon absorptions and particle collisions, it already implements
                         * Eq. 2.17 of Guhathakurtha & Draine, in events/grain/s */
                        /* >>chng 00 mar 27, factored in hden (in Phi), by PvH */
                        /* >>chng 00 mar 29, add in contribution due to particle collisions, by PvH */
                        /* >>chng 01 mar 30, moved multiplication of bval_jk with gv.bin[nd]->cnv_CM3_pGR
                         *   out of loop, PvH */
                        trap2 = p[j]*bval_jk;
                        /* Trapezoidal rule, multiplication with factor 0.5 is done outside loop */
                        sum += (trap1 + trap2)*delu[j];
                        trap1 = trap2;
                }

                /* >>chng 00 mar 27, multiplied with delu, by PvH */
                /* >>chng 00 apr 05, taken out Lambda[0], improves convergence at low end dramatically!, by PvH */
                /* qprob[k] = sum*gv.bin[nd]->cnv_CM3_pGR*delu[k]/(Lambda[k] - Lambda[0]); */
                /* this expression includes factor 0.5 from trapezoidal rule above */
                /* p[k] = 0.5*(sum + (trap1 + p[k]*Phi[0])*delu[k])/Lambda[k] */
                p[k] = (sum + trap1*delu[k])/(2.*Lambda[k] - Phi[0]*delu[k]);

                // total failure -> force next step to be smaller
                if( p[k] <= 0. )
                        return 3.*QHEAT_TOL;
        }

        /* this is estimate for p[k] using one double step of size "step" */
        p2k = (sum2 + trap12*step)/(2.*Lambda[k] - Phi[0]*step);

        // total failure -> force next step to be smaller
        if( p2k <= 0. )
                return 3.*QHEAT_TOL;

        RelErrPk = fabs(p2k-p[k])/p[k];

        /* this is radiative cooling due to the two probability bins we just added */
        /* simple trapezoidal rule will not do here, RelErrCool would never converge */
        *cooling = log_integral(u1[k-2],p[k-2]*Lambda[k-2],u1[k-1],p[k-1]*Lambda[k-1]);
        *cooling += log_integral(u1[k-1],p[k-1]*Lambda[k-1],u1[k],p[k]*Lambda[k]);

        /* same as cooling, but now for double step of size "step" */
        cooling2 = log_integral(u1[k-2],p[k-2]*Lambda[k-2],u1[k],p2k*Lambda[k]);

        /* p[0] is not reliable, so ignore convergence test on cooling on first step */
        RelErrCool = ( index > 0 ) ? fabs(cooling2-(*cooling))/(*cooling) : 0.;

/*      printf( " TryDoubleStep p[k-1] %.4e p[k] %.4e p2k %.4e\n",p[k-1],p[k],p2k ); */
        /* error scales as O(step^3), so this is relative accuracy of p[k] or cooling */
        return MAX2(RelErrPk,RelErrCool)/3.;
}


/* calculate logarithmic integral from (xx1,yy1) to (xx2,yy2) */
STATIC double log_integral(double xx1,
                           double yy1,
                           double xx2,
                           double yy2)
{
        double eps,
          result,
          xx;

        DEBUG_ENTRY( "log_integral()" );

        /* sanity checks */
        ASSERT( xx1 > 0. && yy1 > 0. && xx2 > 0. && yy2 > 0. );

        xx = log(xx2/xx1);
        eps = log((xx2/xx1)*(yy2/yy1));
        if( fabs(eps) < 1.e-4 )
        {
                result = xx1*yy1*xx*((eps/6. + 0.5)*eps + 1.);
        }
        else
        {
                result = (xx2*yy2 - xx1*yy1)*xx/eps;
        }
        return result;
}


/* scan the probability distribution for valid range */
STATIC void ScanProbDistr(double u1[],      /* u1[nbin] */
                          double dPdlnT[],  /* dPdlnT[nbin] */
                          long nbin,
                          double maxVal,
                          long nmax,
                          double qtmin1,
                          /*@out@*/long *nstart,
                          /*@out@*/long *nstart2,
                          /*@out@*/long *nend,
                          long *nWideFail,
                          QH_Code *ErrorCode)
{
        bool lgSetLo,
          lgSetHi;
        long i;
        double deriv_max,
          minVal;
        const double MIN_FAC_LO = 1.e4;
        const double MIN_FAC_HI = 1.e4;

        DEBUG_ENTRY( "ScanProbDistr()" );

        /* sanity checks */
        ASSERT( nbin > 0 && nmax >= 0 && nmax < nbin && maxVal > 0. );

        /* sometimes the probability distribution will start falling before settling on
         * a rising slope. In such a case nstart will point to the first rising point,
         * while nstart2 will point to the point with the steepest derivative on the
         * rising slope. The code will use the distribution from nstart to nend as a
         * valid probability distribution, but the will use the points near nstart2
         * to extrapolate a new value for qtmin if needed */
        minVal = maxVal;
        *nstart = nmax;
        for( i=nmax; i >= 0; --i )
        {
                if( dPdlnT[i] < minVal )
                {
                        *nstart = i;
                        minVal = dPdlnT[i];
                }
        }
        deriv_max = 0.;
        *nstart2 = nmax;
        for( i=nmax; i > *nstart; --i )
        {
                double deriv = log(dPdlnT[i]/dPdlnT[i-1])/log(u1[i]/u1[i-1]);
                if( deriv > deriv_max )
                {
                        *nstart2 = i-1;
                        deriv_max = deriv;
                }
        }
        *nend = nbin-1;

        /* now do quality control; these checks are more stringent than the ones in GetProbDistr_LowLimit */
        lgSetLo = ( nmax >= *nend || maxVal/dPdlnT[*nend] < MIN_FAC_HI );
        /* >>chng 03 jan 22, prevent problems if both dPdlnT and its derivative are continuously rising,
         *                   in which case both lgSetLo and lgSetHi are set and QH_WIDE_FAIL is triggered;
         *                   this can happen if qtmin is far too low; triggered by pahtest.in, PvH */
        if( lgSetLo )
                /* use relaxed test if lgSetLo is already set */
                lgSetHi = ( nmax <= *nstart || maxVal/dPdlnT[*nstart] < MIN_FAC_LO );
        else
                lgSetHi = ( nmax <= *nstart2 || maxVal/dPdlnT[*nstart2] < MIN_FAC_LO );

        if( lgSetLo && lgSetHi )
        {
                ++(*nWideFail);

                if( *nWideFail >= WIDE_FAIL_MAX )
                        *ErrorCode = MAX2(*ErrorCode,QH_WIDE_FAIL);
        }

        if( lgSetLo )
                *ErrorCode = MAX2(*ErrorCode,QH_LOW_FAIL);

        /* if dPdlnT[nstart] is too high, but qtmin1 is already close to GRAIN_TMIN,
         * then don't bother signaling a QH_HIGH_FAIL. grains below GRAIN_TMIN have the
         * peak of their thermal emission beyond 3 meter, so they really are irrelevant
         * since free-free emission from electrons will drown this grain emission... */
        if( lgSetHi && qtmin1 > 1.2*GRAIN_TMIN )
                *ErrorCode = MAX2(*ErrorCode,QH_HIGH_FAIL);

        /* there are insufficient bins to attempt rebinning */
        if( *ErrorCode < QH_NO_REBIN && (*nend - *nstart) < NQMIN ) 
                *ErrorCode = MAX2(*ErrorCode,QH_NBIN_FAIL);

        if( trace.lgTrace && trace.lgDustBug )
        {
                fprintf( ioQQQ, "    ScanProbDistr nstart %ld nstart2 %ld nend %ld nmax %ld maxVal %.3e",
                         *nstart,*nstart2,*nend,nmax,maxVal );
                fprintf( ioQQQ, " dPdlnT[nstart] %.3e dPdlnT[nstart2] %.3e dPdlnT[nend] %.3e code %d\n",
                         dPdlnT[*nstart],dPdlnT[*nstart2],dPdlnT[*nend],*ErrorCode );
        }

        if( *ErrorCode >= QH_NO_REBIN )
        {
                *nstart = -1;
                *nstart2 = -1;
                *nend = -2;
        }
        return;
}


/* rebin the quantum heating results to speed up RT_diffuse */
STATIC long RebinQHeatResults(long nd,
                              long nstart,
                              long nend,
                              double p[],
                              double qtemp[],
                              double qprob[],
                              double dPdlnT[],
                              double u1[],
                              double delu[],
                              double Lambda[],
                              QH_Code *ErrorCode)
{
        long i,
          newnbin;
        double fac,
          help,
          mul_fac,
          *new_delu/*[NQGRID]*/,
          *new_dPdlnT/*[NQGRID]*/,
          *new_Lambda/*[NQGRID]*/,
          *new_p/*[NQGRID]*/,
          *new_qprob/*[NQGRID]*/,
          *new_qtemp/*[NQGRID]*/,
          *new_u1/*[NQGRID]*/,
          PP1,
          PP2,
          RadCooling,
          T1,
          T2,
          Ucheck,
          uu1,
          uu2;

        DEBUG_ENTRY( "RebinQHeatResults()" );

        /* sanity checks */
        ASSERT( nd >= 0 && nd < gv.nBin );
        /* >>chng 02 aug 07, changed oldnbin -> nstart..nend */
        ASSERT( nstart >= 0 && nstart < nend && nend < NQGRID );

        /* leading entries may have become very small or zero -> skip */
        for( i=nstart; i <= nend && dPdlnT[i] < PROB_CUTOFF_LO; i++ ) {}

        /* >>chng 04 oct 17, add fail-safe to keep lint happy, but this should never happen... */
        if( i >= NQGRID )
        {
                *ErrorCode = MAX2(*ErrorCode,QH_REBIN_FAIL);
                return 0;
        }

        /* >>chng 02 aug 15, use malloc to prevent stack overflows */
        new_delu = (double*)MALLOC((size_t)(NQGRID*sizeof(double)));
        new_dPdlnT = (double*)MALLOC((size_t)(NQGRID*sizeof(double)));
        new_Lambda = (double*)MALLOC((size_t)(NQGRID*sizeof(double)));
        new_p = (double*)MALLOC((size_t)(NQGRID*sizeof(double)));
        new_qprob = (double*)MALLOC((size_t)(NQGRID*sizeof(double)));
        new_qtemp = (double*)MALLOC((size_t)(NQGRID*sizeof(double)));
        new_u1 = (double*)MALLOC((size_t)(NQGRID*sizeof(double)));

        newnbin = 0;

        T1 = qtemp[i];
        PP1 = p[i];
        uu1 = u1[i];

        /* >>chng 04 feb 01, change 2.*NQMIN -> 1.5*NQMIN, PvH */
        help = pow(qtemp[nend]/qtemp[i],1./(1.5*NQMIN));
        mul_fac = MIN2(QT_RATIO,help);

        Ucheck = u1[i];
        RadCooling = 0.;

        while( i < nend )
        {
                bool lgBoundErr;
                bool lgDone= false;
                double s0 = 0.;
                double s1 = 0.;
                double wid = 0.;
                double xx,y;

                T2 = T1*mul_fac;

                do 
                {
                        double p1,p2,L1,L2,frac,slope;
                        if( qtemp[i] <= T1 && T1 <= qtemp[i+1] )
                        {
                                /* >>chng 01 nov 15, copy uu2 into uu1 instead, PvH */
                                /* uu1 = ufunct(T1,nd); */
                                frac = log(T1/qtemp[i]);
                                slope = log(p[i+1]/p[i])/log(qtemp[i+1]/qtemp[i]);
                                p1 = p[i]*exp(frac*slope);
                                slope = log(Lambda[i+1]/Lambda[i])/log(qtemp[i+1]/qtemp[i]);
                                L1 = Lambda[i]*exp(frac*slope);
                        }
                        else
                        {
                                /* >>chng 01 nov 15, copy uu2 into uu1 instead, PvH */
                                /* uu1 = u1[i]; */
                                p1 = p[i];
                                L1 = Lambda[i];
                        }
                        if( qtemp[i] <= T2 && T2 <= qtemp[i+1] )
                        {
                                /* >>chng 02 apr 30, make sure this doesn't point beyond valid range, PvH */
                                help = ufunct(T2,nd,&lgBoundErr);
                                uu2 = MIN2(help,u1[i+1]);
                                ASSERT( !lgBoundErr ); /* this should never be triggered */
                                frac = log(T2/qtemp[i]);
                                slope = log(p[i+1]/p[i])/log(qtemp[i+1]/qtemp[i]);
                                p2 = p[i]*exp(frac*slope);
                                slope = log(Lambda[i+1]/Lambda[i])/log(qtemp[i+1]/qtemp[i]);
                                L2 = Lambda[i]*exp(frac*slope);
                                lgDone = true;
                        }
                        else
                        {
                                uu2 = u1[i+1];
                                p2 = p[i+1];
                                L2 = Lambda[i+1];
                                /* >>chng 01 nov 15, this caps the range in p(U) integrated in one bin
                                 * it helps avoid spurious QH_BOUND_FAIL's when flank is very steep, PvH */
                                if( MAX2(p2,PP1)/MIN2(p2,PP1) > sqrt(SAFETY) )
                                {
                                        lgDone = true;
                                        T2 = qtemp[i+1];
                                }
                                ++i;
                        }
                        PP2 = p2;
                        wid += uu2 - uu1;
                        /* sanity check */
                        ASSERT( wid >= 0. );
                        s0 += log_integral(uu1,p1,uu2,p2);
                        s1 += log_integral(uu1,p1*L1,uu2,p2*L2);
                        uu1 = uu2;

                } while( i < nend && ! lgDone );

                /* >>chng 01 nov 14, if T2 == qtemp[oldnbin-1], the code will try another iteration
                 * break here to avoid zero divide, the assert on Ucheck tests if we are really finished */
                /* >>chng 01 dec 04, change ( s0 == 0. ) to ( s0 <= 0. ), PvH */
                if( s0 <= 0. )
                {
                        ASSERT( wid == 0. );
                        break;
                }

                new_qprob[newnbin] = s0;
                new_Lambda[newnbin] = s1/s0;
                xx = log(new_Lambda[newnbin]*EN1RYD*gv.bin[nd]->cnv_GR_pH);
                splint_safe(gv.bin[nd]->dstems,gv.dsttmp,gv.bin[nd]->dstslp,NDEMS,xx,&y,&lgBoundErr);
                ASSERT( !lgBoundErr ); /* this should never be triggered */
                new_qtemp[newnbin] = exp(y);
                new_u1[newnbin] = ufunct(new_qtemp[newnbin],nd,&lgBoundErr);
                ASSERT( !lgBoundErr ); /* this should never be triggered */
                new_delu[newnbin] = wid;
                new_p[newnbin] = new_qprob[newnbin]/new_delu[newnbin];
                new_dPdlnT[newnbin] = new_p[newnbin]*new_qtemp[newnbin]*uderiv(new_qtemp[newnbin],nd);

                Ucheck += wid;
                RadCooling += new_qprob[newnbin]*new_Lambda[newnbin];

                T1 = T2;
                PP1 = PP2;
                ++newnbin;
        }

        /* >>chng 01 jul 13, add fail-safe */
        if( newnbin < NQMIN )
        {
                *ErrorCode = MAX2(*ErrorCode,QH_REBIN_FAIL);

                free(new_delu);
                free(new_dPdlnT);
                free(new_Lambda);
                free(new_p);
                free(new_qprob);
                free(new_qtemp);
                free(new_u1);
                return 0;
        }

        fac = RadCooling*EN1RYD*gv.bin[nd]->cnv_GR_pCM3/gv.bin[nd]->GrainHeat;

        if( trace.lgTrace && trace.lgDustBug )
        {
                fprintf( ioQQQ, "     RebinQHeatResults found tol1 %.4e tol2 %.4e\n",
                         fabs(u1[nend]/Ucheck-1.), fabs(fac-1.) );
        }

        /* do quality control */
        /* >>chng 02 apr 30, tighten up check, PvH */
        ASSERT( fabs(u1[nend]/Ucheck-1.) < 10.*sqrt((double)(nend-nstart+newnbin))*DBL_EPSILON );

        if( fabs(fac-1.) > CONSERV_TOL )
                *ErrorCode = MAX2(*ErrorCode,QH_CONV_FAIL);

        for( i=0; i < newnbin; i++ )
        {
                /* renormalize the distribution to assure energy conservation */
                p[i] = new_p[i]/fac;
                qtemp[i] = new_qtemp[i];
                qprob[i] = new_qprob[i]/fac;
                dPdlnT[i] = new_dPdlnT[i]/fac;
                u1[i] = new_u1[i];
                delu[i] = new_delu[i];
                Lambda[i] = new_Lambda[i];

                /* sanity checks */
                ASSERT( qtemp[i] > 0. && qprob[i] > 0. );

/*              printf(" rk %ld T[k] %.6e U[k] %.6e p[k] %.6e dPdlnT[k] %.6e\n",i,qtemp[i],u1[i],p[i],dPdlnT[i]); */
        }

        free(new_delu);
        free(new_dPdlnT);
        free(new_Lambda);
        free(new_p);
        free(new_qprob);
        free(new_qtemp);
        free(new_u1);
        return newnbin;
}


/* calculate approximate probability distribution in high intensity limit */
STATIC void GetProbDistr_HighLimit(long nd,
                                   double TolFac,
                                   double Umax,
                                   double fwhm,
                                   /*@out@*/double qtemp[],
                                   /*@out@*/double qprob[],
                                   /*@out@*/double dPdlnT[],
                                   /*@out@*/double *tol,
                                   /*@out@*/long *qnbin,
                                   /*@out@*/double *new_tmin,
                                   /*@out@*/QH_Code *ErrorCode)
{
        bool lgBoundErr,
          lgErr;
        long i,
          nbin;
        double c1,
          c2,
          delu[NQGRID],
          fac,
          fac1,
          fac2,
          help1,
          help2,
          L1,
          L2,
          Lambda[NQGRID],
          mul_fac,
          p[NQGRID],
          p1,
          p2,
          RadCooling,
          sum,
          T1,
          T2,
          Tlo,
          Thi,
          Ulo,
          Uhi,
          uu1,
          uu2,
          xx,
          y;

        DEBUG_ENTRY( "GetProbDistr_HighLimit()" );

        if( trace.lgTrace && trace.lgDustBug )
        {
                fprintf( ioQQQ, "   GetProbDistr_HighLimit called for grain %s\n", gv.bin[nd]->chDstLab );
        }

        c1 = sqrt(4.*LN_TWO/PI)/fwhm*exp(-POW2(fwhm/Umax)/(16.*LN_TWO));
        c2 = 4.*LN_TWO*POW2(Umax/fwhm);

        fac1 = fwhm/Umax*sqrt(-log(PROB_CUTOFF_LO)/(4.*LN_TWO));
        /* >>chng 03 nov 10, safeguard against underflow, PvH */
        help1 = Umax*exp(-fac1);
        help2 = exp(gv.bin[nd]->DustEnth[0]);
        Ulo = MAX2(help1,help2);
        /* >>chng 03 jan 28, ignore lgBoundErr on lower boundary, low-T grains have negigible emission, PvH */
        Tlo = inv_ufunct(Ulo,nd,&lgBoundErr);

        fac2 = fwhm/Umax*sqrt(-log(PROB_CUTOFF_HI)/(4.*LN_TWO));
        /* >>chng 03 nov 10, safeguard against overflow, PvH */
        if( fac2 > log(DBL_MAX/10.) )
        {
                *ErrorCode = MAX2(*ErrorCode,QH_WIDE_FAIL);
                return;
        }
        Uhi = Umax*exp(fac2);
        Thi = inv_ufunct(Uhi,nd,&lgBoundErr);

        nbin = 0;

        T1 = Tlo;
        uu1 = ufunct(T1,nd,&lgErr);
        lgBoundErr = lgBoundErr || lgErr;
        help1 = log(uu1/Umax);
        p1 = c1*exp(-c2*POW2(help1));
        splint_safe(gv.dsttmp,gv.bin[nd]->dstems,gv.bin[nd]->dstslp2,NDEMS,log(T1),&y,&lgErr);
        lgBoundErr = lgBoundErr || lgErr;
        L1 = exp(y)*gv.bin[nd]->cnv_H_pGR/EN1RYD;

        /* >>chng 03 nov 10, safeguard against underflow, PvH */
        if( uu1*p1*L1 < 1.e5*DBL_MIN )
        {
                *ErrorCode = MAX2(*ErrorCode,QH_WIDE_FAIL);
                return;
        }

        /* >>chng 04 feb 01, change 2.*NQMIN -> 1.2*NQMIN, PvH */
        help1 = pow(Thi/Tlo,1./(1.2*NQMIN));
        mul_fac = MIN2(QT_RATIO,help1);

        sum = 0.;
        RadCooling = 0.;

        do 
        {
                double s0,s1,wid;

                T2 = T1*mul_fac;
                uu2 = ufunct(T2,nd,&lgErr);
                lgBoundErr = lgBoundErr || lgErr;
                help1 = log(uu2/Umax);
                p2 = c1*exp(-c2*POW2(help1));
                splint_safe(gv.dsttmp,gv.bin[nd]->dstems,gv.bin[nd]->dstslp2,NDEMS,log(T2),&y,&lgErr);
                lgBoundErr = lgBoundErr || lgErr;
                L2 = exp(y)*gv.bin[nd]->cnv_H_pGR/EN1RYD;

                wid = uu2 - uu1;
                s0 = log_integral(uu1,p1,uu2,p2);
                s1 = log_integral(uu1,p1*L1,uu2,p2*L2);

                qprob[nbin] = s0;
                Lambda[nbin] = s1/s0;
                xx = log(Lambda[nbin]*EN1RYD*gv.bin[nd]->cnv_GR_pH);
                splint_safe(gv.bin[nd]->dstems,gv.dsttmp,gv.bin[nd]->dstslp,NDEMS,xx,&y,&lgErr);
                lgBoundErr = lgBoundErr || lgErr;
                qtemp[nbin] = exp(y);
                delu[nbin] = wid;
                p[nbin] = qprob[nbin]/delu[nbin];
                dPdlnT[nbin] = p[nbin]*qtemp[nbin]*uderiv(qtemp[nbin],nd);

                sum += qprob[nbin];
                RadCooling += qprob[nbin]*Lambda[nbin];

                T1 = T2;
                uu1 = uu2;
                p1 = p2;
                L1 = L2;

                ++nbin;

        } while( T2 < Thi && nbin < NQGRID );

        fac = RadCooling*EN1RYD*gv.bin[nd]->cnv_GR_pCM3/gv.bin[nd]->GrainHeat;

        for( i=0; i < nbin; ++i )
        {
                qprob[i] /= fac;
                dPdlnT[i] /= fac;
        }

        *tol = sum/fac;
        *qnbin = nbin;
        *new_tmin = qtemp[0];
        *ErrorCode = MAX2(*ErrorCode,QH_ANALYTIC);

        /* do quality control */
        if( TolFac > STRICT )
                *ErrorCode = MAX2(*ErrorCode,QH_ANALYTIC_RELAX);

        if( lgBoundErr )
                *ErrorCode = MAX2(*ErrorCode,QH_THIGH_FAIL);

        if( fabs(sum/fac-1.) > PROB_TOL )
                *ErrorCode = MAX2(*ErrorCode,QH_CONV_FAIL);

        if( dPdlnT[0] > SAFETY*PROB_CUTOFF_LO || dPdlnT[nbin-1] > SAFETY*PROB_CUTOFF_HI )
                *ErrorCode = MAX2(*ErrorCode,QH_BOUND_FAIL);

        if( trace.lgTrace && trace.lgDustBug )
        {
                fprintf( ioQQQ, "     GetProbDistr_HighLimit found tol1 %.4e tol2 %.4e\n",
                         fabs(sum-1.), fabs(sum/fac-1.) );
                fprintf( ioQQQ, "    zone %ld %s nbin %ld total prob %.4e new_tmin %.4e\n",
                         nzone,gv.bin[nd]->chDstLab,nbin,sum/fac,*new_tmin );
        }
        return;
}


/* calculate derivative of the enthalpy function dU/dT (aka the specific heat) at a given temperature, in Ryd/K */
STATIC double uderiv(double temp, 
                     long int nd)
{
        enth_type ecase;
        long int i,
          j;
        double N_C,
          N_H;
        double deriv = 0.,
          hok[3] = {1275., 1670., 4359.},
          numer,
          dnumer,
          denom,
          ddenom,
          x;


        DEBUG_ENTRY( "uderiv()" );

        if( temp <= 0. ) 
        {
                fprintf( ioQQQ, " uderiv called with non-positive temperature: %.6e\n" , temp );
                cdEXIT(EXIT_FAILURE);
        }
        ASSERT( nd >= 0 && nd < gv.nBin );

        ecase = gv.which_enth[gv.bin[nd]->matType];
        switch( ecase )
        {
        case ENTH_CAR:
                numer = (4.15e-22/EN1RYD)*pow(temp,3.3);
                dnumer = (3.3*4.15e-22/EN1RYD)*pow(temp,2.3);
                denom = 1. + 6.51e-03*temp + 1.5e-06*temp*temp + 8.3e-07*pow(temp,2.3);
                ddenom = 6.51e-03 + 2.*1.5e-06*temp + 2.3*8.3e-07*pow(temp,1.3);
                /* dU/dT for pah/graphitic grains in Ryd/K, derived from:
                 * >>refer      grain   physics Guhathakurta & Draine, 1989, ApJ, 345, 230 */
                deriv = (dnumer*denom - numer*ddenom)/POW2(denom);
                break;
        case ENTH_CAR2:
                /* dU/dT for graphite grains in Ryd/K, using eq 9 of */
                /* >>refer      grain   physics Draine B.T., and Li A., 2001, ApJ, 551, 807 */
                deriv = (DebyeDeriv(temp/863.,2) + 2.*DebyeDeriv(temp/2504.,2))*BOLTZMANN/EN1RYD;
                break;
        case ENTH_SIL:
                /* dU/dT for silicate grains (and grey grains) in Ryd/K */
                /* limits of tlim set above, 0 and DBL_MAX, so always OK */
                /* >>refer      grain   physics Guhathakurta & Draine, 1989, ApJ, 345, 230 */
                for( j = 0; j < 4; j++ )
                {
                        if( temp > tlim[j] && temp <= tlim[j+1] )
                        {
                                deriv = cval[j]*pow(temp,ppower[j]);
                                break;
                        }
                }
                break;
        case ENTH_SIL2:
                /* dU/dT for silicate grains in Ryd/K, using eq 11 of */
                /* >>refer      grain   physics Draine B.T., and Li A., 2001, ApJ, 551, 807 */
                deriv = (2.*DebyeDeriv(temp/500.,2) + DebyeDeriv(temp/1500.,3))*BOLTZMANN/EN1RYD;
                break;
        case ENTH_PAH:
                /* dU/dT for PAH grains in Ryd/K, using eq A.4 of */
                /* >>refer      grain   physics Dwek E., Arendt R.G., Fixsen D.J. et al., 1997, ApJ, 475, 565 */
                /* this expression is only valid upto 2000K */
                x = log10(MIN2(temp,2000.));
                deriv = pow(10.,-21.26+3.1688*x-0.401894*POW2(x))/EN1RYD;
                break;
        case ENTH_PAH2:
                /* dU/dT for PAH grains in Ryd/K, approximately using eq 33 of */
                /* >>refer      grain   physics Draine B.T., and Li A., 2001, ApJ, 551, 807 */
                /* N_C and N_H should actually be nint(N_C) and nint(N_H),
                 * but this can lead to FP overflow for very large grains */
                N_C = NO_ATOMS(nd);
                if( N_C <= 25. )
                {
                        N_H = 0.5*N_C;
                }
                else if( N_C <= 100. )
                {
                        N_H = 2.5*sqrt(N_C);
                }
                else
                {
                        N_H = 0.25*N_C;
                }
                deriv = 0.;
                for( i=0; i < 3; i++ )
                {
                        double help1 = hok[i]/temp;
                        if( help1 < 300. )
                        {
                                double help2 = exp(help1);
                                double help3 = ( help1 < 1.e-7 ) ? help1*(1.+0.5*help1) : help2-1.;
                                deriv += N_H/(N_C-2.)*POW2(help1)*help2/POW2(help3)*BOLTZMANN/EN1RYD;
                        }
                }
                deriv += (DebyeDeriv(temp/863.,2) + 2.*DebyeDeriv(temp/2504.,2))*BOLTZMANN/EN1RYD;
                break;
        default:
                fprintf( ioQQQ, " uderiv called with unknown type for enthalpy function: %d\n", ecase );
                cdEXIT(EXIT_FAILURE);
        }

        /* >>chng 00 mar 23, use formula 3.1 of Guhathakurtha & Draine, by PvH */
        /* >>chng 03 jan 17, use MAX2(..,1) to prevent crash for extremely small grains, PvH */
        deriv *= MAX2(NO_ATOMS(nd)-2.,1.);

        if( deriv <= 0. ) 
        {
                fprintf( ioQQQ, " uderiv finds non-positive derivative: %.6e, what's up?\n" , deriv );
                cdEXIT(EXIT_FAILURE);
        }
        return( deriv );
}


/* calculate the enthalpy of a grain at a given temperature, in Ryd */
STATIC double ufunct(double temp, 
                     long int nd,
                     /*@out@*/ bool *lgBoundErr)
{
        double enthalpy,
          y;

        DEBUG_ENTRY( "ufunct()" );

        if( temp <= 0. ) 
        {
                fprintf( ioQQQ, " ufunct called with non-positive temperature: %.6e\n" , temp );
                cdEXIT(EXIT_FAILURE);
        }
        ASSERT( nd >= 0 && nd < gv.nBin );

        /* >>chng 02 apr 22, interpolate in DustEnth array to get enthalpy, by PvH */
        splint_safe(gv.dsttmp,gv.bin[nd]->DustEnth,gv.bin[nd]->EnthSlp,NDEMS,log(temp),&y,lgBoundErr);
        enthalpy = exp(y);

        ASSERT( enthalpy > 0. );
        return( enthalpy );
}


/* this is the inverse of ufunct: determine grain temperature as a function of enthalpy */
STATIC double inv_ufunct(double enthalpy, 
                         long int nd,
                         /*@out@*/ bool *lgBoundErr)
{
        double temp,
          y;

        DEBUG_ENTRY( "inv_ufunct()" );

        if( enthalpy <= 0. ) 
        {
                fprintf( ioQQQ, " inv_ufunct called with non-positive enthalpy: %.6e\n" , enthalpy );
                cdEXIT(EXIT_FAILURE);
        }
        ASSERT( nd >= 0 && nd < gv.nBin );

        /* >>chng 02 apr 22, interpolate in DustEnth array to get temperature, by PvH */
        splint_safe(gv.bin[nd]->DustEnth,gv.dsttmp,gv.bin[nd]->EnthSlp2,NDEMS,log(enthalpy),&y,lgBoundErr);
        temp = exp(y);

        ASSERT( temp > 0. );
        return( temp );
}


/* initialize interpolation arrys for grain enthalpy */
void InitEnthalpy(void)
{
        double C_V1,
          C_V2,
          tdust1,
          tdust2;
        long int i,
          j,
          nd;

        DEBUG_ENTRY( "InitEnthalpy()" );

        for( nd=0; nd < gv.nBin; nd++ )
        {
                tdust2 = GRAIN_TMIN;
                C_V2 = uderiv(tdust2,nd);
                /* at low temps, C_V = C*T^3 -> U = C*T^4/4 = C_V*T/4 */
                gv.bin[nd]->DustEnth[0] = C_V2*tdust2/4.;
                tdust1 = tdust2;
                C_V1 = C_V2;

                for( i=1; i < NDEMS; i++ )
                {
                        double tmid,Cmid;
                        tdust2 = exp(gv.dsttmp[i]);
                        C_V2 = uderiv(tdust2,nd);
                        tmid = sqrt(tdust1*tdust2);
                        /* this ensures accuracy for silicate enthalpy */
                        for( j=1; j < 4; j++ )
                        {
                                if( tdust1 < tlim[j] && tlim[j] < tdust2 )
                                {
                                        tmid = tlim[j];
                                        break;
                                }
                        }
                        Cmid = uderiv(tmid,nd);
                        gv.bin[nd]->DustEnth[i] = gv.bin[nd]->DustEnth[i-1] +
                                log_integral(tdust1,C_V1,tmid,Cmid) +
                                log_integral(tmid,Cmid,tdust2,C_V2);
                        tdust1 = tdust2;
                        C_V1 = C_V2;
                }
        }

        /* conversion for logarithmic interpolation */
        for( nd=0; nd < gv.nBin; nd++ )
        {
                for( i=0; i < NDEMS; i++ )
                {
                        gv.bin[nd]->DustEnth[i] = log(gv.bin[nd]->DustEnth[i]);
                }
        }

        /* now find slopes from spline fit */
        for( nd=0; nd < gv.nBin; nd++ )
        {
                /* set up coefficients for splint */
                spline(gv.dsttmp,gv.bin[nd]->DustEnth,NDEMS,2e31,2e31,gv.bin[nd]->EnthSlp);
                spline(gv.bin[nd]->DustEnth,gv.dsttmp,NDEMS,2e31,2e31,gv.bin[nd]->EnthSlp2);
        }
        return;
}


/* helper function for calculating specific heat, uses Debye theory */
STATIC double DebyeDeriv(double x,
                         long n)
{
        long i,
          nn;
        double res,
          *xx,
          *rr,
          *aa,
          *ww;

        DEBUG_ENTRY( "DebyeDeriv()" );

        ASSERT( x > 0. );
        ASSERT( n == 2 || n == 3 );

        if( x < 0.001 )
        {
                /* for general n this is Gamma(n+2)*zeta(n+1)*powi(x,n) */
                if( n == 2 )
                {
                        res = 6.*1.202056903159594*POW2(x);
                }
                else if( n == 3 )
                {
                        res = 24.*1.082323233711138*POW3(x);
                }
                else
                        /* added to keep lint happy - note that assert above confimred that n is 2 or 3,
                         * but lint flagged possible flow without defn of res */
                        TotalInsanity();
        }
        else
        {
                nn = 4*MAX2(4,2*(long)(0.05/x));
                xx = (double *)MALLOC(sizeof(double)*(unsigned)nn);
                rr = (double *)MALLOC(sizeof(double)*(unsigned)nn);
                aa = (double *)MALLOC(sizeof(double)*(unsigned)nn);
                ww = (double *)MALLOC(sizeof(double)*(unsigned)nn);
                gauss_legendre(nn,xx,aa);
                gauss_init(nn,0.,1.,xx,aa,rr,ww);

                res = 0.;
                for( i=0; i < nn; i++ )
                {
                        double help1 = rr[i]/x;
                        if( help1 < 300. )
                        {
                                double help2 = exp(help1);
                                double help3 = ( help1 < 1.e-7 ) ? help1*(1.+0.5*help1) : help2-1.;
                                res += ww[i]*powi(rr[i],n+1)*help2/POW2(help3);
                        }
                }
                res /= POW2(x);

                free(ww);
                free(aa);
                free(rr);
                free(xx);
        }
        return (double)n*res;
}

---