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geant4/examples/extended/electromagnetic/TestEm7/src/G4ScreenedNuclearRecoil.cc
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Gabriele Cosmo e2d2f9810a Import Geant4 9.6.0 source tree
2016-06-09 17:01:34 +02:00

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//
// ********************************************************************
// * License and Disclaimer *
// * *
// * The Geant4 software is copyright of the Copyright Holders of *
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// * regarding this software system or assume any liability for its *
// * use. Please see the license in the file LICENSE and URL above *
// * for the full disclaimer and the limitation of liability. *
// * *
// * This code implementation is the result of the scientific and *
// * technical work of the GEANT4 collaboration. *
// * By using, copying, modifying or distributing the software (or *
// * any work based on the software) you agree to acknowledge its *
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// ********************************************************************
//
/// \file electromagnetic/TestEm7/src/G4ScreenedNuclearRecoil.cc
/// \brief Implementation of the G4ScreenedNuclearRecoil class
//
//
// G4ScreenedNuclearRecoil.cc,v 1.57 2008/05/07 11:51:26 marcus Exp
// GEANT4 tag
//
//
// Class Description
// Process for screened electromagnetic nuclear elastic scattering;
// Physics comes from:
// Marcus H. Mendenhall and Robert A. Weller,
// "Algorithms for the rapid computation of classical cross
// sections for screened Coulomb collisions "
// Nuclear Instruments and Methods in Physics Research B58 (1991) 11-17
// The only input required is a screening function phi(r/a) which is the ratio
// of the actual interatomic potential for two atoms with atomic numbers Z1 and Z2,
// to the unscreened potential Z1*Z2*e^2/r where e^2 is elm_coupling in Geant4 units
//
// First version, April 2004, Marcus H. Mendenhall, Vanderbilt University
//
// 5 May, 2004, Marcus Mendenhall
// Added an option for enhancing hard collisions statistically, to allow
// backscattering calculations to be carried out with much improved event rates,
// without distorting the multiple-scattering broadening too much.
// the method SetCrossSectionHardening(G4double fraction, G4double HardeningFactor)
// sets what fraction of the events will be randomly hardened,
// and the factor by which the impact area is reduced for such selected events.
//
// 21 November, 2004, Marcus Mendenhall
// added static_nucleus to IsApplicable
//
// 7 December, 2004, Marcus Mendenhall
// changed mean free path of stopping particle from 0.0 to 1.0*nanometer
// to avoid new verbose warning about 0 MFP in 4.6.2p02
//
// 17 December, 2004, Marcus Mendenhall
// added code to permit screening out overly close collisions which are
// expected to be hadronic, not Coulombic
//
// 19 December, 2004, Marcus Mendenhall
// massive rewrite to add modular physics stages and plug-in cross section table
// computation. This allows one to select (e.g.) between the normal external python
// process and an embedded python interpreter (which is much faster) for generating
// the tables.
// It also allows one to switch between sub-sampled scattering (event biasing) and
// normal scattering, and between non-relativistic kinematics and relativistic
// kinematic approximations, without having a class for every combination. Further, one can
// add extra stages to the scattering, which can implement various book-keeping processes.
//
// January 2007, Marcus Mendenhall
// Reorganized heavily for inclusion in Geant4 Core. All modules merged into
// one source and header, all historic code removed.
//
// Class Description - End
#include <stdio.h>
#include "globals.hh"
#include "G4ScreenedNuclearRecoil.hh"
const char* G4ScreenedCoulombCrossSectionInfo::CVSFileVers() { return
"G4ScreenedNuclearRecoil.cc,v 1.57 2008/05/07 11:51:26 marcus Exp GEANT4 tag ";
}
#include "G4ParticleTypes.hh"
#include "G4ParticleTable.hh"
#include "G4VParticleChange.hh"
#include "G4ParticleChangeForLoss.hh"
#include "G4DataVector.hh"
#include "G4Track.hh"
#include "G4Step.hh"
#include "G4Material.hh"
#include "G4Element.hh"
#include "G4Isotope.hh"
#include "G4MaterialCutsCouple.hh"
#include "G4ElementVector.hh"
#include "G4IsotopeVector.hh"
#include "G4EmProcessSubType.hh"
#include "G4RangeTest.hh"
#include "G4ParticleDefinition.hh"
#include "G4DynamicParticle.hh"
#include "G4ProcessManager.hh"
#include "G4StableIsotopes.hh"
#include "G4LindhardPartition.hh"
#include "G4PhysicalConstants.hh"
#include "G4SystemOfUnits.hh"
#include "Randomize.hh"
#include <iostream>
#include <iomanip>
#include "c2_factory.hh"
static c2_factory<G4double> c2; // this makes a lot of notation shorter
typedef c2_ptr<G4double> c2p;
G4ScreenedCoulombCrossSection::~G4ScreenedCoulombCrossSection()
{
screeningData.clear();
MFPTables.clear();
}
const G4double G4ScreenedCoulombCrossSection::massmap[nMassMapElements+1]={
0, 1.007940, 4.002602, 6.941000, 9.012182, 10.811000, 12.010700,
14.006700, 15.999400, 18.998403, 20.179700, 22.989770, 24.305000, 26.981538, 28.085500,
30.973761, 32.065000, 35.453000, 39.948000, 39.098300, 40.078000, 44.955910, 47.867000,
50.941500, 51.996100, 54.938049, 55.845000, 58.933200, 58.693400, 63.546000, 65.409000,
69.723000, 72.640000, 74.921600, 78.960000, 79.904000, 83.798000, 85.467800, 87.620000,
88.905850, 91.224000, 92.906380, 95.940000, 98.000000, 101.070000, 102.905500, 106.420000,
107.868200, 112.411000, 114.818000, 118.710000, 121.760000, 127.600000, 126.904470, 131.293000,
132.905450, 137.327000, 138.905500, 140.116000, 140.907650, 144.240000, 145.000000, 150.360000,
151.964000, 157.250000, 158.925340, 162.500000, 164.930320, 167.259000, 168.934210, 173.040000,
174.967000, 178.490000, 180.947900, 183.840000, 186.207000, 190.230000, 192.217000, 195.078000,
196.966550, 200.590000, 204.383300, 207.200000, 208.980380, 209.000000, 210.000000, 222.000000,
223.000000, 226.000000, 227.000000, 232.038100, 231.035880, 238.028910, 237.000000, 244.000000,
243.000000, 247.000000, 247.000000, 251.000000, 252.000000, 257.000000, 258.000000, 259.000000,
262.000000, 261.000000, 262.000000, 266.000000, 264.000000, 277.000000, 268.000000, 281.000000,
272.000000, 285.000000, 282.500000, 289.000000, 287.500000, 292.000000};
G4ParticleDefinition* G4ScreenedCoulombCrossSection::SelectRandomUnweightedTarget(const G4MaterialCutsCouple* couple)
{
// Select randomly an element within the material, according to number density only
const G4Material* material = couple->GetMaterial();
G4int nMatElements = material->GetNumberOfElements();
const G4ElementVector* elementVector = material->GetElementVector();
const G4Element *element=0;
G4ParticleDefinition*target=0;
// Special case: the material consists of one element
if (nMatElements == 1)
{
element= (*elementVector)[0];
}
else
{
// Composite material
G4double random = G4UniformRand() * material->GetTotNbOfAtomsPerVolume();
G4double nsum=0.0;
const G4double *atomDensities=material->GetVecNbOfAtomsPerVolume();
for (G4int k=0 ; k < nMatElements ; k++ )
{
nsum+=atomDensities[k];
element= (*elementVector)[k];
if (nsum >= random) break;
}
}
G4int N=0;
G4int Z=(G4int)std::floor(element->GetZ()+0.5);
G4int nIsotopes=element->GetNumberOfIsotopes();
if(!nIsotopes) {
if(Z<=92) {
// we have no detailed material isotopic info available,
// so use G4StableIsotopes table up to Z=92
static G4StableIsotopes theIso; // get a stable isotope table for default results
nIsotopes=theIso.GetNumberOfIsotopes(Z);
G4double random = 100.0*G4UniformRand(); // values are expressed as percent, sum is 100
G4int tablestart=theIso.GetFirstIsotope(Z);
G4double asum=0.0;
for(G4int i=0; i<nIsotopes; i++) {
asum+=theIso.GetAbundance(i+tablestart);
N=theIso.GetIsotopeNucleonCount(i+tablestart);
if(asum >= random) break;
}
} else {
// too heavy for stable isotope table, just use mean mass
N=(G4int)std::floor(element->GetN()+0.5);
}
} else {
G4int i;
const G4IsotopeVector *isoV=element->GetIsotopeVector();
G4double random = G4UniformRand();
G4double *abundance=element->GetRelativeAbundanceVector();
G4double asum=0.0;
for(i=0; i<nIsotopes; i++) {
asum+=abundance[i];
N=(*isoV)[i]->GetN();
if(asum >= random) break;
}
}
// get the official definition of this nucleus, to get the correct value of A
// note that GetIon is very slow, so we will cache ones we have already found ourselves.
ParticleCache::iterator p=targetMap.find(Z*1000+N);
if (p != targetMap.end()) {
target=(*p).second;
} else{
target=G4ParticleTable::GetParticleTable()->GetIon(Z, N, 0.0);
targetMap[Z*1000+N]=target;
}
return target;
}
void G4ScreenedCoulombCrossSection::BuildMFPTables()
{
const G4int nmfpvals=200;
std::vector<G4double> evals(nmfpvals), mfpvals(nmfpvals);
// sum up inverse MFPs per element for each material
const G4MaterialTable* materialTable = G4Material::GetMaterialTable();
if (materialTable == 0) { return; }
//G4Exception("G4ScreenedCoulombCrossSection::BuildMFPTables - no MaterialTable found)");
G4int nMaterials = G4Material::GetNumberOfMaterials();
for (G4int matidx=0; matidx < nMaterials; matidx++) {
const G4Material* material= (*materialTable)[matidx];
const G4ElementVector &elementVector = *(material->GetElementVector());
const G4int nMatElements = material->GetNumberOfElements();
const G4Element *element=0;
const G4double *atomDensities=material->GetVecNbOfAtomsPerVolume();
G4double emin=0, emax=0; // find innermost range of cross section functions
for (G4int kel=0 ; kel < nMatElements ; kel++ )
{
element=elementVector[kel];
G4int Z=(G4int)std::floor(element->GetZ()+0.5);
const G4_c2_function &ifunc=sigmaMap[Z];
if(!kel || ifunc.xmin() > emin) emin=ifunc.xmin();
if(!kel || ifunc.xmax() < emax) emax=ifunc.xmax();
}
G4double logint=std::log(emax/emin) / (nmfpvals-1) ; // logarithmic increment for tables
// compute energy scale for interpolator. Force exact values at both ends to avoid range errors
for (G4int i=1; i<nmfpvals-1; i++) evals[i]=emin*std::exp(logint*i);
evals.front()=emin;
evals.back()=emax;
// zero out the inverse mfp sums to start
for (G4int eidx=0; eidx < nmfpvals; eidx++) mfpvals[eidx] = 0.0;
// sum inverse mfp for each element in this material and for each energy
for (G4int kel=0 ; kel < nMatElements ; kel++ )
{
element=elementVector[kel];
G4int Z=(G4int)std::floor(element->GetZ()+0.5);
const G4_c2_function &sigma=sigmaMap[Z];
G4double ndens = atomDensities[kel]; // compute atom fraction for this element in this material
for (G4int eidx=0; eidx < nmfpvals; eidx++) {
mfpvals[eidx] += ndens*sigma(evals[eidx]);
}
}
// convert inverse mfp to regular mfp
for (G4int eidx=0; eidx < nmfpvals; eidx++) {
mfpvals[eidx] = 1.0/mfpvals[eidx];
}
// and make a new interpolating function out of the sum
MFPTables[matidx] = c2.log_log_interpolating_function().load(evals, mfpvals,true,0,true,0);
}
}
G4ScreenedNuclearRecoil::
G4ScreenedNuclearRecoil(const G4String& processName,
const G4String &ScreeningKey,
G4bool GenerateRecoils,
G4double RecoilCutoff, G4double PhysicsCutoff) :
G4VDiscreteProcess(processName),
screeningKey(ScreeningKey),
generateRecoils(GenerateRecoils), avoidReactions(1),
recoilCutoff(RecoilCutoff), physicsCutoff(PhysicsCutoff),
hardeningFraction(0.0), hardeningFactor(1.0),
externalCrossSectionConstructor(0),
NIELPartitionFunction(new G4LindhardRobinsonPartition)
{
// for now, point to class instance of this. Doing it by creating a new one fails
// to correctly update NIEL
// not even this is needed... done in G4VProcess().
// pParticleChange=&aParticleChange;
processMaxEnergy=50000.0*MeV;
highEnergyLimit=100.0*MeV;
lowEnergyLimit=physicsCutoff;
registerDepositedEnergy=1; // by default, don't hide NIEL
MFPScale=1.0;
// SetVerboseLevel(2);
AddStage(new G4ScreenedCoulombClassicalKinematics);
AddStage(new G4SingleScatter);
SetProcessSubType(fCoulombScattering);
}
void G4ScreenedNuclearRecoil::ResetTables()
{
std::map<G4int, G4ScreenedCoulombCrossSection*>::iterator xt=crossSectionHandlers.begin();
for(;xt != crossSectionHandlers.end(); xt++) {
delete (*xt).second;
}
crossSectionHandlers.clear();
}
void G4ScreenedNuclearRecoil::ClearStages()
{
// I don't think I like deleting the processes here... they are better abandoned
// if the creator doesn't get rid of them
// std::vector<G4ScreenedCollisionStage *>::iterator stage=collisionStages.begin();
//for(; stage != collisionStages.end(); stage++) delete (*stage);
collisionStages.clear();
}
void G4ScreenedNuclearRecoil::SetNIELPartitionFunction(const G4VNIELPartition *part)
{
if(NIELPartitionFunction) delete NIELPartitionFunction;
NIELPartitionFunction=part;
}
void G4ScreenedNuclearRecoil::DepositEnergy(G4int z1, G4double a1, const G4Material *material, G4double energy)
{
if(!NIELPartitionFunction) {
IonizingLoss+=energy;
} else {
G4double part=NIELPartitionFunction->PartitionNIEL(z1, a1, material, energy);
IonizingLoss+=energy*(1-part);
NIEL += energy*part;
}
}
G4ScreenedNuclearRecoil::~G4ScreenedNuclearRecoil()
{
ResetTables();
}
// returns true if it appears the nuclei collided, and we are interested in checking
G4bool G4ScreenedNuclearRecoil::CheckNuclearCollision(
G4double A, G4double a1, G4double apsis) {
return avoidReactions && (apsis < (1.1*(std::pow(A,1.0/3.0)+std::pow(a1,1.0/3.0)) + 1.4)*fermi);
// nuclei are within 1.4 fm (reduced pion Compton wavelength) of each other at apsis,
// this is hadronic, skip it
}
G4ScreenedCoulombCrossSection *G4ScreenedNuclearRecoil::GetNewCrossSectionHandler(void) {
G4ScreenedCoulombCrossSection *xc;
if(!externalCrossSectionConstructor) xc=new G4NativeScreenedCoulombCrossSection;
else xc=externalCrossSectionConstructor->create();
xc->SetVerbosity(verboseLevel);
return xc;
}
G4double G4ScreenedNuclearRecoil::GetMeanFreePath(const G4Track& track,
G4double,
G4ForceCondition* cond)
{
const G4DynamicParticle* incoming = track.GetDynamicParticle();
G4double energy = incoming->GetKineticEnergy();
G4double a1=incoming->GetDefinition()->GetPDGMass()/amu_c2;
G4double meanFreePath;
*cond=NotForced;
if (energy < lowEnergyLimit || energy < recoilCutoff*a1) {
*cond=Forced;
return 1.0*nm; /* catch and stop slow particles to collect their NIEL! */
} else if (energy > processMaxEnergy*a1) {
return DBL_MAX; // infinite mean free path
} else if (energy > highEnergyLimit*a1) energy=highEnergyLimit*a1; /* constant MFP at high energy */
G4double fz1=incoming->GetDefinition()->GetPDGCharge();
G4int z1=(G4int)(fz1/eplus + 0.5);
std::map<G4int, G4ScreenedCoulombCrossSection*>::iterator xh=
crossSectionHandlers.find(z1);
G4ScreenedCoulombCrossSection *xs;
if (xh==crossSectionHandlers.end()) {
xs =crossSectionHandlers[z1]=GetNewCrossSectionHandler();
xs->LoadData(screeningKey, z1, a1, physicsCutoff);
xs->BuildMFPTables();
} else xs=(*xh).second;
const G4MaterialCutsCouple* materialCouple = track.GetMaterialCutsCouple();
size_t materialIndex = materialCouple->GetMaterial()->GetIndex();
const G4_c2_function &mfp=*(*xs)[materialIndex];
// make absolutely certain we don't get an out-of-range energy
meanFreePath = mfp(std::min(std::max(energy, mfp.xmin()), mfp.xmax()));
// G4cout << "MFP: " << meanFreePath << " index " << materialIndex << " energy " << energy << " MFPScale " << MFPScale << G4endl;
return meanFreePath*MFPScale;
}
G4VParticleChange* G4ScreenedNuclearRecoil::PostStepDoIt(const G4Track& aTrack, const G4Step& aStep)
{
validCollision=1;
pParticleChange->Initialize(aTrack);
NIEL=0.0; // default is no NIEL deposited
IonizingLoss=0.0;
// do universal setup
const G4DynamicParticle* incidentParticle = aTrack.GetDynamicParticle();
G4ParticleDefinition *baseParticle=aTrack.GetDefinition();
G4double fz1=baseParticle->GetPDGCharge()/eplus;
G4int z1=(G4int)(fz1+0.5);
G4double a1=baseParticle->GetPDGMass()/amu_c2;
G4double incidentEnergy = incidentParticle->GetKineticEnergy();
// Select randomly one element and (possibly) isotope in the current material.
const G4MaterialCutsCouple* couple = aTrack.GetMaterialCutsCouple();
const G4Material* mat = couple->GetMaterial();
G4double P=0.0; // the impact parameter of this collision
if(incidentEnergy < GetRecoilCutoff()*a1) { // check energy sanity on entry
DepositEnergy(z1, baseParticle->GetPDGMass()/amu_c2, mat, incidentEnergy);
GetParticleChange().ProposeEnergy(0.0);
// stop the particle and bail out
validCollision=0;
} else {
G4double numberDensity=mat->GetTotNbOfAtomsPerVolume();
G4double lattice=0.5/std::pow(numberDensity,1.0/3.0); // typical lattice half-spacing
G4double length=GetCurrentInteractionLength();
G4double sigopi=1.0/(CLHEP::pi*numberDensity*length); // this is sigma0/pi
// compute the impact parameter very early, so if is rejected as too far away, little effort is wasted
// this is the TRIM method for determining an impact parameter based on the flight path
// this gives a cumulative distribution of N(P)= 1-exp(-pi P^2 n l)
// which says the probability of NOT hitting a disk of area sigma= pi P^2 =exp(-sigma N l)
// which may be reasonable
if(sigopi < lattice*lattice) {
// normal long-flight approximation
P = std::sqrt(-std::log(G4UniformRand()) *sigopi);
} else {
// short-flight limit
P = std::sqrt(G4UniformRand())*lattice;
}
G4double fraction=GetHardeningFraction();
if(fraction && G4UniformRand() < fraction) {
// pick out some events, and increase the central cross section
// by reducing the impact parameter
P /= std::sqrt(GetHardeningFactor());
}
// check if we are far enough away that the energy transfer must be below cutoff,
// and leave everything alone if so, saving a lot of time.
if(P*P > sigopi) {
if(GetVerboseLevel() > 1)
printf("ScreenedNuclear impact reject: length=%.3f P=%.4f limit=%.4f\n",
length/angstrom, P/angstrom,std::sqrt(sigopi)/angstrom);
// no collision, don't follow up with anything
validCollision=0;
}
}
// find out what we hit, and record it in our kinematics block.
kinematics.targetMaterial=mat;
kinematics.a1=a1;
if(validCollision) {
G4ScreenedCoulombCrossSection *xsect=GetCrossSectionHandlers()[z1];
G4ParticleDefinition *recoilIon=
xsect->SelectRandomUnweightedTarget(couple);
kinematics.crossSection=xsect;
kinematics.recoilIon=recoilIon;
kinematics.impactParameter=P;
kinematics.a2=recoilIon->GetPDGMass()/amu_c2;
} else {
kinematics.recoilIon=0;
kinematics.impactParameter=0;
kinematics.a2=0;
}
std::vector<G4ScreenedCollisionStage *>::iterator stage=collisionStages.begin();
for(; stage != collisionStages.end(); stage++)
(*stage)->DoCollisionStep(this,aTrack, aStep);
if(registerDepositedEnergy) {
pParticleChange->ProposeLocalEnergyDeposit(IonizingLoss+NIEL);
pParticleChange->ProposeNonIonizingEnergyDeposit(NIEL);
//MHM G4cout << "depositing energy, total = " << IonizingLoss+NIEL << " NIEL = " << NIEL << G4endl;
}
return G4VDiscreteProcess::PostStepDoIt( aTrack, aStep );
}
G4ScreenedCoulombClassicalKinematics::G4ScreenedCoulombClassicalKinematics() :
// instantiate all the needed functions statically, so no allocation is done at run time
// we will be solving x^2 - x phi(x*au)/eps - beta^2 == 0.0
// or, for easier scaling, x'^2 - x' au phi(x')/eps - beta^2 au^2
// note that only the last of these gets deleted, since it owns the rest
phifunc(c2.const_plugin_function()),
xovereps(c2.linear(0., 0., 0.)), // will fill this in with the right slope at run time
diff(c2.quadratic(0., 0., 0., 1.)-xovereps*phifunc)
{
}
G4bool G4ScreenedCoulombClassicalKinematics::DoScreeningComputation(G4ScreenedNuclearRecoil *master,
const G4ScreeningTables *screen, G4double eps, G4double beta)
{
G4double au=screen->au;
G4CoulombKinematicsInfo &kin=master->GetKinematics();
G4double A=kin.a2;
G4double a1=kin.a1;
G4double xx0; // first estimate of closest approach
if(eps < 5.0) {
G4double y=std::log(eps);
G4double mlrho4=((((3.517e-4*y+1.401e-2)*y+2.393e-1)*y+2.734)*y+2.220);
G4double rho4=std::exp(-mlrho4); // W&M eq. 18
G4double bb2=0.5*beta*beta;
xx0=std::sqrt(bb2+std::sqrt(bb2*bb2+rho4)); // W&M eq. 17
} else {
G4double ee=1.0/(2.0*eps);
xx0=ee+std::sqrt(ee*ee+beta*beta); // W&M eq. 15 (Rutherford value)
if(master->CheckNuclearCollision(A, a1, xx0*au)) return 0; // nuclei too close
}
// we will be solving x^2 - x phi(x*au)/eps - beta^2 == 0.0
// or, for easier scaling, x'^2 - x' au phi(x')/eps - beta^2 au^2
xovereps.reset(0., 0.0, au/eps); // slope of x*au/eps term
phifunc.set_function(&(screen->EMphiData.get())); // install interpolating table
G4double xx1, phip, phip2;
G4int root_error;
xx1=diff->find_root(phifunc.xmin(), std::min(10*xx0*au,phifunc.xmax()),
std::min(xx0*au, phifunc.xmax()), beta*beta*au*au, &root_error, &phip, &phip2)/au;
if(root_error) {
G4cout << "Screened Coulomb Root Finder Error" << G4endl;
G4cout << "au " << au << " A " << A << " a1 " << a1 << " xx1 " << xx1 << " eps " << eps << " beta " << beta << G4endl;
G4cout << " xmin " << phifunc.xmin() << " xmax " << std::min(10*xx0*au,phifunc.xmax()) ;
G4cout << " f(xmin) " << phifunc(phifunc.xmin()) << " f(xmax) " << phifunc(std::min(10*xx0*au,phifunc.xmax())) ;
G4cout << " xstart " << std::min(xx0*au, phifunc.xmax()) << " target " << beta*beta*au*au ;
G4cout << G4endl;
throw c2_exception("Failed root find");
}
// phiprime is scaled by one factor of au because phi is evaluated at (xx0*au),
G4double phiprime=phip*au;
//lambda0 is from W&M 19
G4double lambda0=1.0/std::sqrt(0.5+beta*beta/(2.0*xx1*xx1)-phiprime/(2.0*eps));
//compute the 6-term Lobatto integral alpha (per W&M 21, with different coefficients)
// this is probably completely un-needed but gives the highest quality results,
G4double alpha=(1.0+ lambda0)/30.0;
G4double xvals[]={0.98302349, 0.84652241, 0.53235309, 0.18347974};
G4double weights[]={0.03472124, 0.14769029, 0.23485003, 0.18602489};
for(G4int k=0; k<4; k++) {
G4double x, ff;
x=xx1/xvals[k];
ff=1.0/std::sqrt(1.0-phifunc(x*au)/(x*eps)-beta*beta/(x*x));
alpha+=weights[k]*ff;
}
phifunc.unset_function(); // throws an exception if used without setting again
G4double thetac1=CLHEP::pi*beta*alpha/xx1; // complement of CM scattering angle
G4double sintheta=std::sin(thetac1); //note sin(pi-theta)=sin(theta)
G4double costheta=-std::cos(thetac1); // note cos(pi-theta)=-cos(theta)
// G4double psi=std::atan2(sintheta, costheta+a1/A); // lab scattering angle (M&T 3rd eq. 8.69)
// numerics note: because we checked above for reasonable values of beta which give real recoils,
// we don't have to look too closely for theta -> 0 here (which would cause sin(theta)
// and 1-cos(theta) to both vanish and make the atan2 ill behaved).
G4double zeta=std::atan2(sintheta, 1-costheta); // lab recoil angle (M&T 3rd eq. 8.73)
G4double coszeta=std::cos(zeta);
G4double sinzeta=std::sin(zeta);
kin.sinTheta=sintheta;
kin.cosTheta=costheta;
kin.sinZeta=sinzeta;
kin.cosZeta=coszeta;
return 1; // all OK, collision is valid
}
void G4ScreenedCoulombClassicalKinematics::DoCollisionStep(G4ScreenedNuclearRecoil *master,
const G4Track& aTrack, const G4Step&) {
if(!master->GetValidCollision()) return;
G4ParticleChange &aParticleChange=master->GetParticleChange();
G4CoulombKinematicsInfo &kin=master->GetKinematics();
const G4DynamicParticle* incidentParticle = aTrack.GetDynamicParticle();
G4ParticleDefinition *baseParticle=aTrack.GetDefinition();
G4double incidentEnergy = incidentParticle->GetKineticEnergy();
// this adjustment to a1 gives the right results for soft (constant gamma)
// relativistic collisions. Hard collisions are wrong anyway, since the
// Coulombic and hadronic terms interfere and cannot be added.
G4double gamma=(1.0+incidentEnergy/baseParticle->GetPDGMass());
G4double a1=kin.a1*gamma; // relativistic gamma correction
G4ParticleDefinition *recoilIon=kin.recoilIon;
G4double A=recoilIon->GetPDGMass()/amu_c2;
G4int Z=(G4int)((recoilIon->GetPDGCharge()/eplus)+0.5);
G4double Ec = incidentEnergy*(A/(A+a1)); // energy in CM frame (non-relativistic!)
const G4ScreeningTables *screen=kin.crossSection->GetScreening(Z);
G4double au=screen->au; // screening length
G4double beta = kin.impactParameter/au; // dimensionless impact parameter
G4double eps = Ec/(screen->z1*Z*elm_coupling/au); // dimensionless energy
G4bool ok=DoScreeningComputation(master, screen, eps, beta);
if(!ok) {
master->SetValidCollision(0); // flag bad collision
return; // just bail out without setting valid flag
}
G4double eRecoil=4*incidentEnergy*a1*A*kin.cosZeta*kin.cosZeta/((a1+A)*(a1+A));
kin.eRecoil=eRecoil;
if(incidentEnergy-eRecoil < master->GetRecoilCutoff()*a1) {
aParticleChange.ProposeEnergy(0.0);
master->DepositEnergy(int(screen->z1), a1, kin.targetMaterial, incidentEnergy-eRecoil);
}
if(master->GetEnableRecoils() && eRecoil > master->GetRecoilCutoff() * kin.a2) {
kin.recoilIon=recoilIon;
} else {
kin.recoilIon=0; // this flags no recoil to be generated
master->DepositEnergy(Z, A, kin.targetMaterial, eRecoil) ;
}
}
void G4SingleScatter::DoCollisionStep(G4ScreenedNuclearRecoil *master,
const G4Track& aTrack, const G4Step&) {
if(!master->GetValidCollision()) return;
G4CoulombKinematicsInfo &kin=master->GetKinematics();
G4ParticleChange &aParticleChange=master->GetParticleChange();
const G4DynamicParticle* incidentParticle = aTrack.GetDynamicParticle();
G4double incidentEnergy = incidentParticle->GetKineticEnergy();
G4double eRecoil=kin.eRecoil;
G4double azimuth=G4UniformRand()*(2.0*CLHEP::pi);
G4double sa=std::sin(azimuth);
G4double ca=std::cos(azimuth);
G4ThreeVector recoilMomentumDirection(kin.sinZeta*ca, kin.sinZeta*sa, kin.cosZeta);
G4ParticleMomentum incidentDirection = incidentParticle->GetMomentumDirection();
recoilMomentumDirection=recoilMomentumDirection.rotateUz(incidentDirection);
G4ThreeVector recoilMomentum=recoilMomentumDirection*std::sqrt(2.0*eRecoil*kin.a2*amu_c2);
if(aParticleChange.GetEnergy() != 0.0) { // DoKinematics hasn't stopped it!
G4ThreeVector beamMomentum=incidentParticle->GetMomentum()-recoilMomentum;
aParticleChange.ProposeMomentumDirection(beamMomentum.unit()) ;
aParticleChange.ProposeEnergy(incidentEnergy-eRecoil);
}
if(kin.recoilIon) {
G4DynamicParticle* recoil = new G4DynamicParticle (kin.recoilIon,
recoilMomentumDirection,eRecoil) ;
aParticleChange.SetNumberOfSecondaries(1);
aParticleChange.AddSecondary(recoil);
}
}
G4bool G4ScreenedNuclearRecoil::
IsApplicable(const G4ParticleDefinition& aParticleType)
{
return aParticleType == *(G4Proton::Proton()) ||
aParticleType.GetParticleType() == "nucleus" ||
aParticleType.GetParticleType() == "static_nucleus";
}
void
G4ScreenedNuclearRecoil::
DumpPhysicsTable(const G4ParticleDefinition&)
{
}
// This used to be the file mhmScreenedNuclearRecoil_native.cc
// it has been included here to collect this file into a smaller number of packages
#include "G4DataVector.hh"
#include "G4Material.hh"
#include "G4Element.hh"
#include "G4Isotope.hh"
#include "G4MaterialCutsCouple.hh"
#include "G4ElementVector.hh"
#include <vector>
G4_c2_function &ZBLScreening(G4int z1, G4int z2, size_t npoints, G4double rMax, G4double *auval)
{
static const size_t ncoef=4;
static G4double scales[ncoef]={-3.2, -0.9432, -0.4028, -0.2016};
static G4double coefs[ncoef]={0.1818,0.5099,0.2802,0.0281};
G4double au=0.8854*angstrom*0.529/(std::pow(z1, 0.23)+std::pow(z2,0.23));
std::vector<G4double> r(npoints), phi(npoints);
for(size_t i=0; i<npoints; i++) {
G4double rr=(float)i/(float)(npoints-1);
r[i]=rr*rr*rMax; // use quadratic r scale to make sampling fine near the center
G4double sum=0.0;
for(size_t j=0; j<ncoef; j++) sum+=coefs[j]*std::exp(scales[j]*r[i]/au);
phi[i]=sum;
}
// compute the derivative at the origin for the spline
G4double phiprime0=0.0;
for(size_t j=0; j<ncoef; j++) phiprime0+=scales[j]*coefs[j]*std::exp(scales[j]*r[0]/au);
phiprime0*=(1.0/au); // put back in natural units;
*auval=au;
return c2.lin_log_interpolating_function().load(r, phi, false, phiprime0,true,0);
}
G4_c2_function &MoliereScreening(G4int z1, G4int z2, size_t npoints, G4double rMax, G4double *auval)
{
static const size_t ncoef=3;
static G4double scales[ncoef]={-6.0, -1.2, -0.3};
static G4double coefs[ncoef]={0.10, 0.55, 0.35};
G4double au=0.8853*0.529*angstrom/std::sqrt(std::pow(z1, 0.6667)+std::pow(z2,0.6667));
std::vector<G4double> r(npoints), phi(npoints);
for(size_t i=0; i<npoints; i++) {
G4double rr=(float)i/(float)(npoints-1);
r[i]=rr*rr*rMax; // use quadratic r scale to make sampling fine near the center
G4double sum=0.0;
for(size_t j=0; j<ncoef; j++) sum+=coefs[j]*std::exp(scales[j]*r[i]/au);
phi[i]=sum;
}
// compute the derivative at the origin for the spline
G4double phiprime0=0.0;
for(size_t j=0; j<ncoef; j++) phiprime0+=scales[j]*coefs[j]*std::exp(scales[j]*r[0]/au);
phiprime0*=(1.0/au); // put back in natural units;
*auval=au;
return c2.lin_log_interpolating_function().load(r, phi, false, phiprime0,true,0);
}
G4_c2_function &LJScreening(G4int z1, G4int z2, size_t npoints, G4double rMax, G4double *auval)
{
//from Loftager, Besenbacher, Jensen & Sorensen
//PhysRev A20, 1443++, 1979
G4double au=0.8853*0.529*angstrom/std::sqrt(std::pow(z1, 0.6667)+std::pow(z2,0.6667));
std::vector<G4double> r(npoints), phi(npoints);
for(size_t i=0; i<npoints; i++) {
G4double rr=(float)i/(float)(npoints-1);
r[i]=rr*rr*rMax; // use quadratic r scale to make sampling fine near the center
G4double y=std::sqrt(9.67*r[i]/au);
G4double ysq=y*y;
G4double phipoly=1+y+0.3344*ysq+0.0485*y*ysq+0.002647*ysq*ysq;
phi[i]=phipoly*std::exp(-y);
// G4cout << r[i] << " " << phi[i] << G4endl;
}
// compute the derivative at the origin for the spline
G4double logphiprime0=(9.67/2.0)*(2*0.3344-1.0); // #avoid 0/0 on first element
logphiprime0 *= (1.0/au); // #put back in natural units
*auval=au;
return c2.lin_log_interpolating_function().load(r, phi, false, logphiprime0*phi[0],true,0);
}
G4_c2_function &LJZBLScreening(G4int z1, G4int z2, size_t npoints, G4double rMax, G4double *auval)
{
// hybrid of LJ and ZBL, uses LJ if x < 0.25*auniv, ZBL if x > 1.5*auniv, and
/// connector in between. These numbers are selected so the switchover
// is very near the point where the functions naturally cross.
G4double auzbl, aulj;
c2p zbl=ZBLScreening(z1, z2, npoints, rMax, &auzbl);
c2p lj=LJScreening(z1, z2, npoints, rMax, &aulj);
G4double au=(auzbl+aulj)*0.5;
lj->set_domain(lj->xmin(), 0.25*au);
zbl->set_domain(1.5*au,zbl->xmax());
c2p conn=c2.connector_function(lj->xmax(), lj, zbl->xmin(), zbl, true,0);
c2_piecewise_function_p<G4double> &pw=c2.piecewise_function();
c2p keepit(pw);
pw.append_function(lj);
pw.append_function(conn);
pw.append_function(zbl);
*auval=au;
keepit.release_for_return();
return pw;
}
G4NativeScreenedCoulombCrossSection::~G4NativeScreenedCoulombCrossSection() {
}
G4NativeScreenedCoulombCrossSection::G4NativeScreenedCoulombCrossSection() {
AddScreeningFunction("zbl", ZBLScreening);
AddScreeningFunction("lj", LJScreening);
AddScreeningFunction("mol", MoliereScreening);
AddScreeningFunction("ljzbl", LJZBLScreening);
}
std::vector<G4String> G4NativeScreenedCoulombCrossSection::GetScreeningKeys() const {
std::vector<G4String> keys;
// find the available screening keys
std::map<std::string, ScreeningFunc>::const_iterator sfunciter=phiMap.begin();
for(; sfunciter != phiMap.end(); sfunciter++) keys.push_back((*sfunciter).first);
return keys;
}
static inline G4double cm_energy(G4double a1, G4double a2, G4double t0) {
// "relativistically correct energy in CM frame"
G4double m1=a1*amu_c2, mass2=a2*amu_c2;
G4double mc2=(m1+mass2);
G4double f=2.0*mass2*t0/(mc2*mc2);
// old way: return (f < 1e-6) ? 0.5*mc2*f : mc2*(std::sqrt(1.0+f)-1.0);
// formally equivalent to previous, but numerically stable for all f without conditional
// uses identity (sqrt(1+x) - 1)(sqrt(1+x) + 1) = x
return mc2*f/(std::sqrt(1.0+f)+1.0);
}
static inline G4double thetac(G4double m1, G4double mass2, G4double eratio) {
G4double s2th2=eratio*( (m1+mass2)*(m1+mass2)/(4.0*m1*mass2) );
G4double sth2=std::sqrt(s2th2);
return 2.0*std::asin(sth2);
}
void G4NativeScreenedCoulombCrossSection::LoadData(G4String screeningKey, G4int z1, G4double a1, G4double recoilCutoff)
{
static const size_t sigLen=200; // since sigma doesn't matter much, a very coarse table will do
G4DataVector energies(sigLen);
G4DataVector data(sigLen);
a1=standardmass(z1); // use standardized values for mass for building tables
const G4MaterialTable* materialTable = G4Material::GetMaterialTable();
if (materialTable == 0) { return; }
//G4Exception("mhmNativeCrossSection::LoadData - no MaterialTable found)");
G4int nMaterials = G4Material::GetNumberOfMaterials();
for (G4int im=0; im<nMaterials; im++)
{
const G4Material* material= (*materialTable)[im];
const G4ElementVector* elementVector = material->GetElementVector();
const G4int nMatElements = material->GetNumberOfElements();
for (G4int iEl=0; iEl<nMatElements; iEl++)
{
G4Element* element = (*elementVector)[iEl];
G4int Z = (G4int) element->GetZ();
G4double a2=element->GetA()*(mole/gram);
if(sigmaMap.find(Z)!=sigmaMap.end()) continue; // we've already got this element
// find the screening function generator we need
std::map<std::string, ScreeningFunc>::iterator sfunciter=phiMap.find(screeningKey);
if(sfunciter==phiMap.end()) {
G4cout << "no such screening key " << screeningKey << G4endl; // FIXME later
exit(1);
}
ScreeningFunc sfunc=(*sfunciter).second;
G4double au;
G4_c2_ptr screen=sfunc(z1, Z, 200, 50.0*angstrom, &au); // generate the screening data
G4ScreeningTables st;
st.EMphiData=screen; //save our phi table
st.z1=z1; st.m1=a1; st.z2=Z; st.m2=a2; st.emin=recoilCutoff;
st.au=au;
// now comes the hard part... build the total cross section tables from the phi table
//based on (pi-thetac) = pi*beta*alpha/x0, but noting that alpha is very nearly unity, always
//so just solve it wth alpha=1, which makes the solution much easier
//this function returns an approximation to (beta/x0)^2=phi(x0)/(eps*x0)-1 ~ ((pi-thetac)/pi)^2
//Since we don't need exact sigma values, this is good enough (within a factor of 2 almost always)
//this rearranges to phi(x0)/(x0*eps) = 2*theta/pi - theta^2/pi^2
c2_linear_p<G4double> &c2eps=c2.linear(0.0, 0.0, 1.0); // will store an appropriate eps inside this in loop
G4_c2_ptr phiau=screen(c2.linear(0.0, 0.0, au));
G4_c2_ptr x0func(phiau/c2eps); // this will be phi(x)/(x*eps) when c2eps is correctly set
x0func->set_domain(1e-6*angstrom/au, 0.9999*screen->xmax()/au); // needed for inverse function
// use the c2_inverse_function interface for the root finder... it is more efficient for an ordered
// computation of values.
G4_c2_ptr x0_solution(c2.inverse_function(x0func));
G4double m1c2=a1*amu_c2;
G4double escale=z1*Z*elm_coupling/au; // energy at screening distance
G4double emax=m1c2; // model is doubtful in very relativistic range
G4double eratkin=0.9999*(4*a1*a2)/((a1+a2)*(a1+a2)); // #maximum kinematic ratio possible at 180 degrees
G4double cmfact0=st.emin/cm_energy(a1, a2, st.emin);
G4double l1=std::log(emax);
G4double l0=std::log(st.emin*cmfact0/eratkin);
if(verbosity >=1)
G4cout << "Native Screening: " << screeningKey << " " << z1 << " " << a1 << " " <<
Z << " " << a2 << " " << recoilCutoff << G4endl;
for(size_t idx=0; idx<sigLen; idx++) {
G4double ee=std::exp(idx*((l1-l0)/sigLen)+l0);
G4double gamma=1.0+ee/m1c2;
G4double eratio=(cmfact0*st.emin)/ee; // factor by which ee needs to be reduced to get emin
G4double theta=thetac(gamma*a1, a2, eratio);
G4double eps=cm_energy(a1, a2, ee)/escale; // #make sure lab energy is converted to CM for these calculations
c2eps.reset(0.0, 0.0, eps); // set correct slope in this function
G4double q=theta/pi;
// G4cout << ee << " " << m1c2 << " " << gamma << " " << eps << " " << theta << " " << q << G4endl;
// old way using root finder
// G4double x0= x0func->find_root(1e-6*angstrom/au, 0.9999*screen.xmax()/au, 1.0, 2*q-q*q);
// new way using c2_inverse_function which caches useful information so should be a bit faster
// since we are scanning this in strict order.
G4double x0=0;
try {
x0=x0_solution(2*q-q*q);
} catch(c2_exception e) {
//G4Exception(G4String("G4ScreenedNuclearRecoil: failure in inverse solution to generate MFP Tables: ")+e.what());
}
G4double betasquared=x0*x0 - x0*phiau(x0)/eps;
G4double sigma=pi*betasquared*au*au;
energies[idx]=ee;
data[idx]=sigma;
}
screeningData[Z]=st;
sigmaMap[Z] = c2.log_log_interpolating_function().load(energies, data, true,0,true,0);
}
}
}
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