| Geant4 Cross Reference |
1 // 1 //
2 // ******************************************* 2 // ********************************************************************
3 // * License and Disclaimer 3 // * License and Disclaimer *
4 // * 4 // * *
5 // * The Geant4 software is copyright of th 5 // * The Geant4 software is copyright of the Copyright Holders of *
6 // * the Geant4 Collaboration. It is provided 6 // * the Geant4 Collaboration. It is provided under the terms and *
7 // * conditions of the Geant4 Software License 7 // * conditions of the Geant4 Software License, included in the file *
8 // * LICENSE and available at http://cern.ch/ 8 // * LICENSE and available at http://cern.ch/geant4/license . These *
9 // * include a list of copyright holders. 9 // * include a list of copyright holders. *
10 // * 10 // * *
11 // * Neither the authors of this software syst 11 // * Neither the authors of this software system, nor their employing *
12 // * institutes,nor the agencies providing fin 12 // * institutes,nor the agencies providing financial support for this *
13 // * work make any representation or warran 13 // * work make any representation or warranty, express or implied, *
14 // * regarding this software system or assum 14 // * regarding this software system or assume any liability for its *
15 // * use. Please see the license in the file 15 // * use. Please see the license in the file LICENSE and URL above *
16 // * for the full disclaimer and the limitatio 16 // * for the full disclaimer and the limitation of liability. *
17 // * 17 // * *
18 // * This code implementation is the result 18 // * This code implementation is the result of the scientific and *
19 // * technical work of the GEANT4 collaboratio 19 // * technical work of the GEANT4 collaboration. *
20 // * By using, copying, modifying or distri 20 // * By using, copying, modifying or distributing the software (or *
21 // * any work based on the software) you ag 21 // * any work based on the software) you agree to acknowledge its *
22 // * use in resulting scientific publicati 22 // * use in resulting scientific publications, and indicate your *
23 // * acceptance of all terms of the Geant4 Sof 23 // * acceptance of all terms of the Geant4 Software license. *
24 // ******************************************* 24 // ********************************************************************
25 // 25 //
26 // 26 //
27 // 27 //
28 // original by H.P. Wellisch << 28 // original by H.P. Wellisch
29 // modified by J.L. Chuma, TRIUMF, 19-Nov-1996 << 29 // modified by J.L. Chuma, TRIUMF, 19-Nov-1996
30 // last modified: 27-Mar-1997 << 30 // last modified: 27-Mar-1997
31 // J.P.Wellisch: 23-Apr-97: minor simplificati << 31 // J.P.Wellisch: 23-Apr-97: minor simplifications
32 // modified by J.L.Chuma 24-Jul-97 to set the << 32 // modified by J.L.Chuma 24-Jul-97 to set the total momentum in Cinema and
33 // Evaporatio << 33 // EvaporationEffects
34 // modified by J.L.Chuma 21-Oct-97 put std::a << 34 // modified by J.L.Chuma 21-Oct-97 put std::abs() around the totalE^2-mass^2
35 // in calcula << 35 // in calculation of total momentum in
36 // Cinema and << 36 // Cinema and EvaporationEffects
37 // Chr. Volcker, 10-Nov-1997: new methods and << 37 // Chr. Volcker, 10-Nov-1997: new methods and class variables.
38 // HPW added utilities for low energy neutron << 38 // HPW added utilities for low energy neutron transport. (12.04.1998)
39 // M.G. Pia, 2 Oct 1998: modified GetFermiMome << 39 // M.G. Pia, 2 Oct 1998: modified GetFermiMomentum to avoid memory leaks
40 // G.Folger, spring 2010: add integer A/Z int << 40 // G.Folger, spring 2010: add integer A/Z interface
41 // A. Ribon, summer 2015: migrated to G4Exp a <<
42 // A. Ribon, autumn 2021: extended to hypernu <<
43 41
44 #include "G4Nucleus.hh" 42 #include "G4Nucleus.hh"
45 #include "G4NucleiProperties.hh" 43 #include "G4NucleiProperties.hh"
46 #include "G4PhysicalConstants.hh" <<
47 #include "G4SystemOfUnits.hh" <<
48 #include "Randomize.hh" 44 #include "Randomize.hh"
49 #include "G4HadronicException.hh" 45 #include "G4HadronicException.hh"
50 #include "G4Exp.hh" << 46
51 #include "G4Log.hh" <<
52 #include "G4HyperNucleiProperties.hh" <<
53 #include "G4HadronicParameters.hh" <<
54 <<
55 <<
56 G4Nucleus::G4Nucleus() 47 G4Nucleus::G4Nucleus()
57 : theA(0), theZ(0), theL(0), aEff(0.0), zEff << 48 : theA(0), theZ(0), aEff(0.0), zEff(0)
58 { 49 {
59 pnBlackTrackEnergy = 0.0; 50 pnBlackTrackEnergy = 0.0;
60 dtaBlackTrackEnergy = 0.0; 51 dtaBlackTrackEnergy = 0.0;
61 pnBlackTrackEnergyfromAnnihilation = 0.0; 52 pnBlackTrackEnergyfromAnnihilation = 0.0;
62 dtaBlackTrackEnergyfromAnnihilation = 0.0; 53 dtaBlackTrackEnergyfromAnnihilation = 0.0;
63 excitationEnergy = 0.0; 54 excitationEnergy = 0.0;
64 momentum = G4ThreeVector(0.,0.,0.); 55 momentum = G4ThreeVector(0.,0.,0.);
65 fermiMomentum = 1.52*hbarc/fermi; 56 fermiMomentum = 1.52*hbarc/fermi;
66 theTemp = 293.16*kelvin; 57 theTemp = 293.16*kelvin;
67 fIsotope = 0; <<
68 } 58 }
69 59
70 G4Nucleus::G4Nucleus( const G4double A, const << 60 G4Nucleus::G4Nucleus( const G4double A, const G4double Z )
71 { 61 {
72 SetParameters( A, Z, std::max(numberOfLambda << 62 SetParameters( A, Z );
73 pnBlackTrackEnergy = 0.0; 63 pnBlackTrackEnergy = 0.0;
74 dtaBlackTrackEnergy = 0.0; 64 dtaBlackTrackEnergy = 0.0;
75 pnBlackTrackEnergyfromAnnihilation = 0.0; 65 pnBlackTrackEnergyfromAnnihilation = 0.0;
76 dtaBlackTrackEnergyfromAnnihilation = 0.0; 66 dtaBlackTrackEnergyfromAnnihilation = 0.0;
77 excitationEnergy = 0.0; 67 excitationEnergy = 0.0;
78 momentum = G4ThreeVector(0.,0.,0.); 68 momentum = G4ThreeVector(0.,0.,0.);
79 fermiMomentum = 1.52*hbarc/fermi; 69 fermiMomentum = 1.52*hbarc/fermi;
80 theTemp = 293.16*kelvin; 70 theTemp = 293.16*kelvin;
81 fIsotope = 0; <<
82 } 71 }
83 72
84 G4Nucleus::G4Nucleus( const G4int A, const G4i << 73 G4Nucleus::G4Nucleus( const G4int A, const G4int Z )
85 { 74 {
86 SetParameters( A, Z, std::max(numberOfLambda << 75 SetParameters( A, Z );
87 pnBlackTrackEnergy = 0.0; 76 pnBlackTrackEnergy = 0.0;
88 dtaBlackTrackEnergy = 0.0; 77 dtaBlackTrackEnergy = 0.0;
89 pnBlackTrackEnergyfromAnnihilation = 0.0; 78 pnBlackTrackEnergyfromAnnihilation = 0.0;
90 dtaBlackTrackEnergyfromAnnihilation = 0.0; 79 dtaBlackTrackEnergyfromAnnihilation = 0.0;
91 excitationEnergy = 0.0; 80 excitationEnergy = 0.0;
92 momentum = G4ThreeVector(0.,0.,0.); 81 momentum = G4ThreeVector(0.,0.,0.);
93 fermiMomentum = 1.52*hbarc/fermi; 82 fermiMomentum = 1.52*hbarc/fermi;
94 theTemp = 293.16*kelvin; 83 theTemp = 293.16*kelvin;
95 fIsotope = 0; <<
96 } 84 }
97 85
98 G4Nucleus::G4Nucleus( const G4Material *aMater 86 G4Nucleus::G4Nucleus( const G4Material *aMaterial )
99 { 87 {
100 ChooseParameters( aMaterial ); 88 ChooseParameters( aMaterial );
101 pnBlackTrackEnergy = 0.0; 89 pnBlackTrackEnergy = 0.0;
102 dtaBlackTrackEnergy = 0.0; 90 dtaBlackTrackEnergy = 0.0;
103 pnBlackTrackEnergyfromAnnihilation = 0.0; 91 pnBlackTrackEnergyfromAnnihilation = 0.0;
104 dtaBlackTrackEnergyfromAnnihilation = 0.0; 92 dtaBlackTrackEnergyfromAnnihilation = 0.0;
105 excitationEnergy = 0.0; 93 excitationEnergy = 0.0;
106 momentum = G4ThreeVector(0.,0.,0.); 94 momentum = G4ThreeVector(0.,0.,0.);
107 fermiMomentum = 1.52*hbarc/fermi; 95 fermiMomentum = 1.52*hbarc/fermi;
108 theTemp = aMaterial->GetTemperature(); 96 theTemp = aMaterial->GetTemperature();
109 fIsotope = 0; <<
110 } 97 }
111 98
112 G4Nucleus::~G4Nucleus() {} 99 G4Nucleus::~G4Nucleus() {}
113 100
114 << 101 G4ReactionProduct G4Nucleus::
115 //-------------------------------------------- << 102 GetBiasedThermalNucleus(G4double aMass, G4ThreeVector aVelocity, G4double temp) const
116 // SVT (Sampling of the Velocity of the Target <<
117 //-------------------------------------------- <<
118 G4ReactionProduct <<
119 G4Nucleus::GetBiasedThermalNucleus(G4double aM <<
120 { 103 {
121 // If E_neutron <= E_threshold, Then apply t << 104 G4double velMag = aVelocity.mag();
122 // Else consider the target nucleus being wi <<
123 G4double E_threshold = G4HadronicParameters: <<
124 if ( E_threshold == -1. ) { <<
125 E_threshold = 400.0*8.617333262E-11*temp; <<
126 } <<
127 G4double E_neutron = 0.5*aVelocity.mag2()*G4 <<
128 <<
129 G4ReactionProduct result; 105 G4ReactionProduct result;
130 result.SetMass(aMass*G4Neutron::Neutron()->G << 106 G4double value = 0;
131 << 107 G4double random = 1;
132 if ( E_neutron <= E_threshold ) { << 108 G4double norm = 3.*std::sqrt(k_Boltzmann*temp*aMass*G4Neutron::Neutron()->GetPDGMass());
133 << 109 norm /= G4Neutron::Neutron()->GetPDGMass();
134 // Beta = sqrt(m/2kT) << 110 norm *= 5.;
135 G4double beta = std::sqrt(result.GetMass() << 111 norm += velMag;
136 << 112 norm /= velMag;
137 // Neutron speed vn << 113 while(value/norm<random)
138 G4double vN_norm = aVelocity.mag(); << 114 {
139 G4double vN_norm2 = vN_norm*vN_norm; << 115 result = GetThermalNucleus(aMass, temp);
140 G4double y = beta*vN_norm; << 116 G4ThreeVector targetVelocity = 1./result.GetMass()*result.GetMomentum();
141 << 117 value = (targetVelocity+aVelocity).mag()/velMag;
142 // Normalize neutron velocity << 118 random = G4UniformRand();
143 aVelocity = (1./vN_norm)*aVelocity; <<
144 <<
145 // Sample target speed <<
146 G4double x2; <<
147 G4double randThreshold; <<
148 G4double vT_norm, vT_norm2, mu; //theta, v <<
149 G4double acceptThreshold; <<
150 G4double vRelativeSpeed; <<
151 G4double cdf0 = 2./(2.+std::sqrt(CLHEP::pi <<
152 <<
153 do { <<
154 // Sample the target velocity vT in the <<
155 if ( G4UniformRand() < cdf0 ) { <<
156 // Sample in C45 from https://laws.lan <<
157 x2 = -std::log(G4UniformRand()*G4Unifo <<
158 } else { <<
159 // Sample in C61 from https://laws.lan <<
160 G4double ampl = std::cos(CLHEP::pi/2.0 <<
161 x2 = -std::log(G4UniformRand()) - std: <<
162 } <<
163 <<
164 vT_norm = std::sqrt(x2)/beta; <<
165 vT_norm2 = vT_norm*vT_norm; <<
166 <<
167 // Sample cosine between the incident ne <<
168 mu = 2*G4UniformRand() - 1; <<
169 <<
170 // Define acceptance threshold <<
171 vRelativeSpeed = std::sqrt(vN_norm2 + vT <<
172 acceptThreshold = vRelativeSpeed/(vN_nor <<
173 randThreshold = G4UniformRand(); <<
174 } while ( randThreshold >= acceptThreshold <<
175 <<
176 DoKinematicsOfThermalNucleus(mu, vT_norm, <<
177 <<
178 } else { // target nucleus considered as bei <<
179 <<
180 result.SetMomentum(0., 0., 0.); <<
181 result.SetKineticEnergy(0.); <<
182 <<
183 } 119 }
184 <<
185 return result; 120 return result;
186 } 121 }
187 122
188 << 123 G4ReactionProduct G4Nucleus::GetThermalNucleus(G4double targetMass, G4double temp) const
189 void << 124 {
190 G4Nucleus::DoKinematicsOfThermalNucleus(const << 125 G4double currentTemp = temp;
191 G4Reac << 126 if(currentTemp < 0) currentTemp = theTemp;
192 << 127 G4ReactionProduct theTarget;
193 // Get target nucleus direction from the neu << 128 theTarget.SetMass(targetMass*G4Neutron::Neutron()->GetPDGMass());
194 G4double cosTh = mu; << 129 G4double px, py, pz;
195 G4ThreeVector uNorm = aVelocity; << 130 px = GetThermalPz(theTarget.GetMass(), currentTemp);
196 << 131 py = GetThermalPz(theTarget.GetMass(), currentTemp);
197 G4double sinTh = std::sqrt(1. - cosTh*cosTh) << 132 pz = GetThermalPz(theTarget.GetMass(), currentTemp);
198 << 133 theTarget.SetMomentum(px, py, pz);
199 // Sample randomly the phi angle between the << 134 G4double tMom = std::sqrt(px*px+py*py+pz*pz);
200 G4double phi = CLHEP::twopi*G4UniformRand(); << 135 G4double tEtot = std::sqrt((tMom+theTarget.GetMass())*
201 G4double sinPhi = std::sin(phi); << 136 (tMom+theTarget.GetMass())-
202 G4double cosPhi = std::cos(phi); << 137 2.*tMom*theTarget.GetMass());
203 << 138 if(1-tEtot/theTarget.GetMass()>0.001)
204 // Find orthogonal vector to aVelocity - sol << 139 {
205 G4ThreeVector ortho(1., 1., 1.); << 140 theTarget.SetTotalEnergy(tEtot);
206 if ( uNorm[0] ) ortho[0] = -(uNorm[1]+ << 141 }
207 else if ( uNorm[1] ) ortho[1] = -(uNorm[0]+ << 142 else
208 else if ( uNorm[2] ) ortho[2] = -(uNorm[0]+ << 143 {
209 << 144 theTarget.SetKineticEnergy(tMom*tMom/(2.*theTarget.GetMass()));
210 // Normalize the vector << 145 }
211 ortho = (1/ortho.mag())*ortho; << 146 return theTarget;
212 <<
213 // Find vector to draw a plan perpendicular <<
214 G4ThreeVector orthoComp( uNorm[1]*ortho[2] - <<
215 uNorm[2]*ortho[0] - <<
216 uNorm[0]*ortho[1] - <<
217 <<
218 // Find the direction of the target velocity <<
219 G4ThreeVector directionTarget( cosTh*uNorm[0 <<
220 cosTh*uNorm[1 <<
221 cosTh*uNorm[2 <<
222 <<
223 // Normalize directionTarget <<
224 directionTarget = ( 1./directionTarget.mag() <<
225 <<
226 // Set momentum <<
227 G4double px = result.GetMass()*vT_norm*direc <<
228 G4double py = result.GetMass()*vT_norm*direc <<
229 G4double pz = result.GetMass()*vT_norm*direc <<
230 result.SetMomentum(px, py, pz); <<
231 <<
232 G4double tMom = std::sqrt(px*px+py*py+pz*pz) <<
233 G4double tEtot = std::sqrt( (tMom+result.Get <<
234 - 2.*tMom*result.GetMass() <<
235 <<
236 if ( tEtot/result.GetMass() - 1. > 0.001 ) { <<
237 // use relativistic energy for higher ener <<
238 result.SetTotalEnergy(tEtot); <<
239 } else { <<
240 // use p**2/2M for lower energies (to pres <<
241 result.SetKineticEnergy(tMom*tMom/(2.*resu <<
242 } 147 }
243 <<
244 } <<
245 <<
246 <<
247 G4ReactionProduct <<
248 G4Nucleus::GetThermalNucleus(G4double targetMa <<
249 { <<
250 G4double currentTemp = temp; <<
251 if (currentTemp < 0) currentTemp = theTemp; <<
252 G4ReactionProduct theTarget; <<
253 theTarget.SetMass(targetMass*G4Neutron::Neut <<
254 G4double px, py, pz; <<
255 px = GetThermalPz(theTarget.GetMass(), curre <<
256 py = GetThermalPz(theTarget.GetMass(), curre <<
257 pz = GetThermalPz(theTarget.GetMass(), curre <<
258 theTarget.SetMomentum(px, py, pz); <<
259 G4double tMom = std::sqrt(px*px+py*py+pz*pz) <<
260 G4double tEtot = std::sqrt((tMom+theTarget.G <<
261 (tMom+theTarget.G <<
262 2.*tMom*theTarge <<
263 // if(1-tEtot/theTarget.GetMass()>0.001) t <<
264 if (tEtot/theTarget.GetMass() - 1. > 0.001) <<
265 // use relativistic energy for higher ener <<
266 theTarget.SetTotalEnergy(tEtot); <<
267 <<
268 } else { <<
269 // use p**2/2M for lower energies (to pres <<
270 theTarget.SetKineticEnergy(tMom*tMom/(2.*t <<
271 } <<
272 return theTarget; <<
273 } <<
274 <<
275 148
276 void << 149 void
277 G4Nucleus::ChooseParameters(const G4Material* << 150 G4Nucleus::ChooseParameters( const G4Material *aMaterial )
278 { << 151 {
279 G4double random = G4UniformRand(); << 152 G4double random = G4UniformRand();
280 G4double sum = aMaterial->GetTotNbOfAtomsPer << 153 G4double sum = aMaterial->GetTotNbOfAtomsPerVolume();
281 const G4ElementVector* theElementVector = aM << 154 const G4ElementVector *theElementVector = aMaterial->GetElementVector();
282 G4double running(0); << 155 G4double running(0);
283 // G4Element* element(0); << 156 G4Element* element(0);
284 const G4Element* element = (*theElementVecto << 157 for(unsigned int i=0; i<aMaterial->GetNumberOfElements(); ++i )
285 << 158 {
286 for (unsigned int i = 0; i < aMaterial->GetN << 159 running += aMaterial->GetVecNbOfAtomsPerVolume()[i];
287 running += aMaterial->GetVecNbOfAtomsPerVo << 160 if( running > random*sum ) {
288 if (running > random*sum) { << 161 element=(*theElementVector)[i];
289 element = (*theElementVector)[i]; << 162 break;
290 break; << 163 }
>> 164 }
>> 165 if ( element->GetNumberOfIsotopes() > 0 ) {
>> 166 G4double randomAbundance = G4UniformRand();
>> 167 G4double sumAbundance = element->GetRelativeAbundanceVector()[0];
>> 168 unsigned int iso=0;
>> 169 while ( iso < element->GetNumberOfIsotopes() &&
>> 170 sumAbundance < randomAbundance ) {
>> 171 ++iso;
>> 172 sumAbundance += element->GetRelativeAbundanceVector()[iso];
>> 173 }
>> 174 theA=element->GetIsotope(iso)->GetN();
>> 175 theZ=element->GetIsotope(iso)->GetZ();
>> 176 aEff=theA;
>> 177 zEff=theZ;
>> 178 } else {
>> 179 aEff = element->GetN();
>> 180 zEff = element->GetZ();
>> 181 theZ = G4int(zEff + 0.5);
>> 182 theA = G4int(aEff + 0.5);
291 } 183 }
292 } 184 }
293 << 185
294 if (element->GetNumberOfIsotopes() > 0) { << 186 void
295 G4double randomAbundance = G4UniformRand() << 187 G4Nucleus::SetParameters( const G4double A, const G4double Z )
296 G4double sumAbundance = element->GetRelati << 188 {
297 unsigned int iso=0; << 189 theZ = G4int(Z + 0.5);
298 while (iso < element->GetNumberOfIsotopes( << 190 theA = G4int(A + 0.5);
299 sumAbundance < randomAbundance) { << 191 if( theA<1 || theZ<0 || theZ>theA )
300 ++iso; << 192 {
301 sumAbundance += element->GetRelativeAbun << 193 throw G4HadronicException(__FILE__, __LINE__,
302 } << 194 "G4Nucleus::SetParameters called with non-physical parameters");
303 theA=element->GetIsotope(iso)->GetN(); << 195 }
304 theZ=element->GetIsotope(iso)->GetZ(); << 196 aEff = A; // atomic weight
305 theL=0; << 197 zEff = Z; // atomic number
306 aEff=theA; <<
307 zEff=theZ; <<
308 } else { <<
309 aEff = element->GetN(); <<
310 zEff = element->GetZ(); <<
311 theZ = G4int(zEff + 0.5); <<
312 theA = G4int(aEff + 0.5); <<
313 theL=0; <<
314 } 198 }
315 } <<
316 <<
317 <<
318 void <<
319 G4Nucleus::SetParameters( const G4double A, co <<
320 { <<
321 theZ = G4lrint(Z); <<
322 theA = G4lrint(A); <<
323 theL = std::max(numberOfLambdas, 0); <<
324 if (theA<1 || theZ<0 || theZ>theA) { <<
325 throw G4HadronicException(__FILE__, __LINE <<
326 "G4Nucleus::SetParameters called w <<
327 } <<
328 aEff = A; // atomic weight <<
329 zEff = Z; // atomic number <<
330 fIsotope = 0; <<
331 } <<
332 <<
333 199
334 void << 200 void
335 G4Nucleus::SetParameters( const G4int A, const << 201 G4Nucleus::SetParameters( const G4int A, const G4int Z )
336 { << 202 {
337 theZ = Z; << 203 theZ = Z;
338 theA = A; << 204 theA = A;
339 theL = std::max(numberOfLambdas, 0); << 205 if( theA<1 || theZ<0 || theZ>theA )
340 if( theA<1 || theZ<0 || theZ>theA ) <<
341 { 206 {
342 throw G4HadronicException(__FILE__, __LI 207 throw G4HadronicException(__FILE__, __LINE__,
343 "G4Nucleus::SetParameters called with << 208 "G4Nucleus::SetParameters called with non-physical parameters");
344 } 209 }
345 aEff = A; // atomic weight << 210 aEff = A; // atomic weight
346 zEff = Z; // atomic number << 211 zEff = Z; // atomic number
347 fIsotope = 0; <<
348 } <<
349 <<
350 <<
351 G4DynamicParticle * <<
352 G4Nucleus::ReturnTargetParticle() const <<
353 { <<
354 // choose a proton or a neutron (or a lamba <<
355 G4DynamicParticle *targetParticle = new G4Dy <<
356 const G4double rnd = G4UniformRand(); <<
357 if ( rnd < zEff/aEff ) { <<
358 targetParticle->SetDefinition( G4Proton::P <<
359 } else if ( rnd < (zEff + theL*1.0)/aEff ) { <<
360 targetParticle->SetDefinition( G4Lambda::L <<
361 } else { <<
362 targetParticle->SetDefinition( G4Neutron:: <<
363 } 212 }
364 return targetParticle; <<
365 } <<
366 213
>> 214 G4DynamicParticle *
>> 215 G4Nucleus::ReturnTargetParticle() const
>> 216 {
>> 217 // choose a proton or a neutron as the target particle
>> 218
>> 219 G4DynamicParticle *targetParticle = new G4DynamicParticle;
>> 220 if( G4UniformRand() < zEff/aEff )
>> 221 targetParticle->SetDefinition( G4Proton::Proton() );
>> 222 else
>> 223 targetParticle->SetDefinition( G4Neutron::Neutron() );
>> 224 return targetParticle;
>> 225 }
367 226
368 G4double << 227 G4double
369 G4Nucleus::AtomicMass( const G4double A, const << 228 G4Nucleus::AtomicMass( const G4double A, const G4double Z ) const
370 { << 229 {
371 // Now returns (atomic mass - electron masse << 230 // Now returns (atomic mass - electron masses)
372 if ( numberOfLambdas > 0 ) { <<
373 return G4HyperNucleiProperties::GetNuclear <<
374 } else { <<
375 return G4NucleiProperties::GetNuclearMass( 231 return G4NucleiProperties::GetNuclearMass(A, Z);
376 } 232 }
377 } <<
378 <<
379 233
380 G4double << 234 G4double
381 G4Nucleus::AtomicMass( const G4int A, const G4 << 235 G4Nucleus::AtomicMass( const G4int A, const G4int Z ) const
382 { << 236 {
383 // Now returns (atomic mass - electron masse << 237 // Now returns (atomic mass - electron masses)
384 if ( numberOfLambdas > 0 ) { <<
385 return G4HyperNucleiProperties::GetNuclear <<
386 } else { <<
387 return G4NucleiProperties::GetNuclearMass( 238 return G4NucleiProperties::GetNuclearMass(A, Z);
388 } 239 }
389 } <<
390 240
>> 241 G4double
>> 242 G4Nucleus::GetThermalPz( const G4double mass, const G4double temp ) const
>> 243 {
>> 244 G4double result = G4RandGauss::shoot();
>> 245 result *= std::sqrt(k_Boltzmann*temp*mass); // Das ist impuls (Pz),
>> 246 // nichtrelativistische rechnung
>> 247 // Maxwell verteilung angenommen
>> 248 return result;
>> 249 }
391 250
392 G4double << 251 G4double
393 G4Nucleus::GetThermalPz( const G4double mass, << 252 G4Nucleus::EvaporationEffects( G4double kineticEnergy )
394 { << 253 {
395 G4double result = G4RandGauss::shoot(); << 254 // derived from original FORTRAN code EXNU by H. Fesefeldt (10-Dec-1986)
396 result *= std::sqrt(k_Boltzmann*temp*mass); << 255 //
397 // ni << 256 // Nuclear evaporation as function of atomic number
398 // Ma << 257 // and kinetic energy (MeV) of primary particle
399 return result; << 258 //
400 } << 259 // returns kinetic energy (MeV)
>> 260 //
>> 261 if( aEff < 1.5 )
>> 262 {
>> 263 pnBlackTrackEnergy = dtaBlackTrackEnergy = 0.0;
>> 264 return 0.0;
>> 265 }
>> 266 G4double ek = kineticEnergy/GeV;
>> 267 G4float ekin = std::min( 4.0, std::max( 0.1, ek ) );
>> 268 const G4float atno = std::min( 120., aEff );
>> 269 const G4float gfa = 2.0*((aEff-1.0)/70.)*std::exp(-(aEff-1.0)/70.);
>> 270 //
>> 271 // 0.35 value at 1 GeV
>> 272 // 0.05 value at 0.1 GeV
>> 273 //
>> 274 G4float cfa = std::max( 0.15, 0.35 + ((0.35-0.05)/2.3)*std::log(ekin) );
>> 275 G4float exnu = 7.716 * cfa * std::exp(-cfa)
>> 276 * ((atno-1.0)/120.)*std::exp(-(atno-1.0)/120.);
>> 277 G4float fpdiv = std::max( 0.5, 1.0-0.25*ekin*ekin );
>> 278 //
>> 279 // pnBlackTrackEnergy is the kinetic energy (in GeV) available for
>> 280 // proton/neutron black track particles
>> 281 // dtaBlackTrackEnergy is the kinetic energy (in GeV) available for
>> 282 // deuteron/triton/alpha black track particles
>> 283 //
>> 284 pnBlackTrackEnergy = exnu*fpdiv;
>> 285 dtaBlackTrackEnergy = exnu*(1.0-fpdiv);
>> 286
>> 287 if( G4int(zEff+0.1) != 82 )
>> 288 {
>> 289 G4double ran1 = -6.0;
>> 290 G4double ran2 = -6.0;
>> 291 for( G4int i=0; i<12; ++i )
>> 292 {
>> 293 ran1 += G4UniformRand();
>> 294 ran2 += G4UniformRand();
>> 295 }
>> 296 pnBlackTrackEnergy *= 1.0 + ran1*gfa;
>> 297 dtaBlackTrackEnergy *= 1.0 + ran2*gfa;
>> 298 }
>> 299 pnBlackTrackEnergy = std::max( 0.0, pnBlackTrackEnergy );
>> 300 dtaBlackTrackEnergy = std::max( 0.0, dtaBlackTrackEnergy );
>> 301 while( pnBlackTrackEnergy+dtaBlackTrackEnergy >= ek )
>> 302 {
>> 303 pnBlackTrackEnergy *= 1.0 - 0.5*G4UniformRand();
>> 304 dtaBlackTrackEnergy *= 1.0 - 0.5*G4UniformRand();
>> 305 }
>> 306 // G4cout << "EvaporationEffects "<<kineticEnergy<<" "
>> 307 // <<pnBlackTrackEnergy+dtaBlackTrackEnergy<<endl;
>> 308 return (pnBlackTrackEnergy+dtaBlackTrackEnergy)*GeV;
>> 309 }
401 310
>> 311 G4double G4Nucleus::AnnihilationEvaporationEffects(G4double kineticEnergy, G4double ekOrg)
>> 312 {
>> 313 // Nuclear evaporation as a function of atomic number and kinetic
>> 314 // energy (MeV) of primary particle. Modified for annihilation effects.
>> 315 //
>> 316 if( aEff < 1.5 || ekOrg < 0.)
>> 317 {
>> 318 pnBlackTrackEnergyfromAnnihilation = 0.0;
>> 319 dtaBlackTrackEnergyfromAnnihilation = 0.0;
>> 320 return 0.0;
>> 321 }
>> 322 G4double ek = kineticEnergy/GeV;
>> 323 G4float ekin = std::min( 4.0, std::max( 0.1, ek ) );
>> 324 const G4float atno = std::min( 120., aEff );
>> 325 const G4float gfa = 2.0*((aEff-1.0)/70.)*std::exp(-(aEff-1.0)/70.);
>> 326
>> 327 G4float cfa = std::max( 0.15, 0.35 + ((0.35-0.05)/2.3)*std::log(ekin) );
>> 328 G4float exnu = 7.716 * cfa * std::exp(-cfa)
>> 329 * ((atno-1.0)/120.)*std::exp(-(atno-1.0)/120.);
>> 330 G4float fpdiv = std::max( 0.5, 1.0-0.25*ekin*ekin );
402 331
403 G4double << 332 pnBlackTrackEnergyfromAnnihilation = exnu*fpdiv;
404 G4Nucleus::EvaporationEffects( G4double kineti << 333 dtaBlackTrackEnergyfromAnnihilation = exnu*(1.0-fpdiv);
405 { << 334
406 // derived from original FORTRAN code EXNU b <<
407 // <<
408 // Nuclear evaporation as function of atomic <<
409 // and kinetic energy (MeV) of primary parti <<
410 // <<
411 // returns kinetic energy (MeV) <<
412 // <<
413 if( aEff < 1.5 ) <<
414 { <<
415 pnBlackTrackEnergy = dtaBlackTrackEnergy = <<
416 return 0.0; <<
417 } <<
418 G4double ek = kineticEnergy/GeV; <<
419 G4float ekin = std::min( 4.0, std::max( 0.1, <<
420 const G4float atno = std::min( 120., aEff ); <<
421 const G4float gfa = 2.0*((aEff-1.0)/70.)*G4E <<
422 // <<
423 // 0.35 value at 1 GeV <<
424 // 0.05 value at 0.1 GeV <<
425 // <<
426 G4float cfa = std::max( 0.15, 0.35 + ((0.35- <<
427 G4float exnu = 7.716 * cfa * G4Exp(-cfa) <<
428 * ((atno-1.0)/120.)*G4Exp(-(atno-1.0)/120. <<
429 G4float fpdiv = std::max( 0.5, 1.0-0.25*ekin <<
430 // <<
431 // pnBlackTrackEnergy is the kinetic energy <<
432 // proton/neutron black <<
433 // dtaBlackTrackEnergy is the kinetic energy <<
434 // deuteron/triton/alpha <<
435 // <<
436 pnBlackTrackEnergy = exnu*fpdiv; <<
437 dtaBlackTrackEnergy = exnu*(1.0-fpdiv); <<
438 <<
439 if( G4int(zEff+0.1) != 82 ) <<
440 { <<
441 G4double ran1 = -6.0; 335 G4double ran1 = -6.0;
442 G4double ran2 = -6.0; 336 G4double ran2 = -6.0;
443 for( G4int i=0; i<12; ++i ) << 337 for( G4int i=0; i<12; ++i ) {
444 { <<
445 ran1 += G4UniformRand(); 338 ran1 += G4UniformRand();
446 ran2 += G4UniformRand(); 339 ran2 += G4UniformRand();
447 } 340 }
448 pnBlackTrackEnergy *= 1.0 + ran1*gfa; << 341 pnBlackTrackEnergyfromAnnihilation *= 1.0 + ran1*gfa;
449 dtaBlackTrackEnergy *= 1.0 + ran2*gfa; << 342 dtaBlackTrackEnergyfromAnnihilation *= 1.0 + ran2*gfa;
450 } <<
451 pnBlackTrackEnergy = std::max( 0.0, pnBlackT <<
452 dtaBlackTrackEnergy = std::max( 0.0, dtaBlac <<
453 while( pnBlackTrackEnergy+dtaBlackTrackEnerg <<
454 { <<
455 pnBlackTrackEnergy *= 1.0 - 0.5*G4UniformR <<
456 dtaBlackTrackEnergy *= 1.0 - 0.5*G4Uniform <<
457 } <<
458 //G4cout << "EvaporationEffects "<<kineticEn <<
459 // <<pnBlackTrackEnergy+dtaBlackTrackE <<
460 return (pnBlackTrackEnergy+dtaBlackTrackEner <<
461 } <<
462 343
463 << 344 pnBlackTrackEnergyfromAnnihilation = std::max( 0.0, pnBlackTrackEnergyfromAnnihilation);
464 G4double << 345 dtaBlackTrackEnergyfromAnnihilation = std::max( 0.0, dtaBlackTrackEnergyfromAnnihilation);
465 G4Nucleus::AnnihilationEvaporationEffects(G4do << 346 G4double blackSum = pnBlackTrackEnergyfromAnnihilation+dtaBlackTrackEnergyfromAnnihilation;
466 { << 347 if (blackSum >= ekOrg/GeV) {
467 // Nuclear evaporation as a function of atom << 348 pnBlackTrackEnergyfromAnnihilation *= ekOrg/GeV/blackSum;
468 // energy (MeV) of primary particle. Modifi << 349 dtaBlackTrackEnergyfromAnnihilation *= ekOrg/GeV/blackSum;
469 // << 350 }
470 if( aEff < 1.5 || ekOrg < 0.) <<
471 { <<
472 pnBlackTrackEnergyfromAnnihilation = 0.0; <<
473 dtaBlackTrackEnergyfromAnnihilation = 0.0; <<
474 return 0.0; <<
475 } <<
476 G4double ek = kineticEnergy/GeV; <<
477 G4float ekin = std::min( 4.0, std::max( 0.1, <<
478 const G4float atno = std::min( 120., aEff ); <<
479 const G4float gfa = 2.0*((aEff-1.0)/70.)*G4E <<
480 <<
481 G4float cfa = std::max( 0.15, 0.35 + ((0.35- <<
482 G4float exnu = 7.716 * cfa * G4Exp(-cfa) <<
483 * ((atno-1.0)/120.)*G4Exp(-(atno-1.0)/120. <<
484 G4float fpdiv = std::max( 0.5, 1.0-0.25*ekin <<
485 <<
486 pnBlackTrackEnergyfromAnnihilation = exnu*fp <<
487 dtaBlackTrackEnergyfromAnnihilation = exnu*( <<
488 <<
489 G4double ran1 = -6.0; <<
490 G4double ran2 = -6.0; <<
491 for( G4int i=0; i<12; ++i ) { <<
492 ran1 += G4UniformRand(); <<
493 ran2 += G4UniformRand(); <<
494 } <<
495 pnBlackTrackEnergyfromAnnihilation *= 1.0 + <<
496 dtaBlackTrackEnergyfromAnnihilation *= 1.0 + <<
497 <<
498 pnBlackTrackEnergyfromAnnihilation = std::ma <<
499 dtaBlackTrackEnergyfromAnnihilation = std::m <<
500 G4double blackSum = pnBlackTrackEnergyfromAn <<
501 if (blackSum >= ekOrg/GeV) { <<
502 pnBlackTrackEnergyfromAnnihilation *= ekOr <<
503 dtaBlackTrackEnergyfromAnnihilation *= ekO <<
504 } <<
505 <<
506 return (pnBlackTrackEnergyfromAnnihilation+d <<
507 } <<
508 351
>> 352 return (pnBlackTrackEnergyfromAnnihilation+dtaBlackTrackEnergyfromAnnihilation)*GeV;
>> 353 }
509 354
510 G4double << 355 G4double
511 G4Nucleus::Cinema( G4double kineticEnergy ) << 356 G4Nucleus::Cinema( G4double kineticEnergy )
512 { << 357 {
513 // derived from original FORTRAN code CINEMA << 358 // derived from original FORTRAN code CINEMA by H. Fesefeldt (14-Oct-1987)
514 // << 359 //
515 // input: kineticEnergy (MeV) << 360 // input: kineticEnergy (MeV)
516 // returns modified kinetic energy (MeV) << 361 // returns modified kinetic energy (MeV)
517 // << 362 //
518 static const G4double expxu = 82.; << 363 static const G4double expxu = 82.; // upper bound for arg. of exp
519 static const G4double expxl = -expxu; << 364 static const G4double expxl = -expxu; // lower bound for arg. of exp
520 << 365
521 G4double ek = kineticEnergy/GeV; << 366 G4double ek = kineticEnergy/GeV;
522 G4double ekLog = G4Log( ek ); << 367 G4double ekLog = std::log( ek );
523 G4double aLog = G4Log( aEff ); << 368 G4double aLog = std::log( aEff );
524 G4double em = std::min( 1.0, 0.2390 + 0.0408 << 369 G4double em = std::min( 1.0, 0.2390 + 0.0408*aLog*aLog );
525 G4double temp1 = -ek * std::min( 0.15, 0.001 << 370 G4double temp1 = -ek * std::min( 0.15, 0.0019*aLog*aLog*aLog );
526 G4double temp2 = G4Exp( std::max( expxl, std << 371 G4double temp2 = std::exp( std::max( expxl, std::min( expxu, -(ekLog-em)*(ekLog-em)*2.0 ) ) );
527 G4double result = 0.0; << 372 G4double result = 0.0;
528 if( std::abs( temp1 ) < 1.0 ) << 373 if( std::abs( temp1 ) < 1.0 )
529 { << 374 {
530 if( temp2 > 1.0e-10 )result = temp1*temp2; << 375 if( temp2 > 1.0e-10 )result = temp1*temp2;
531 } << 376 }
532 else result = temp1*temp2; << 377 else result = temp1*temp2;
533 if( result < -ek )result = -ek; << 378 if( result < -ek )result = -ek;
534 return result*GeV; << 379 return result*GeV;
535 } << 380 }
536 381
>> 382 //
>> 383 // methods for class G4Nucleus ... by Christian Volcker
>> 384 //
537 385
538 G4ThreeVector G4Nucleus::GetFermiMomentum() << 386 G4ThreeVector G4Nucleus::GetFermiMomentum()
539 { << 387 {
540 // chv: .. we assume zero temperature! << 388 // chv: .. we assume zero temperature!
541 << 389
542 // momentum is equally distributed in each p << 390 // momentum is equally distributed in each phasespace volume dpx, dpy, dpz.
543 G4double ranflat1= << 391 G4double ranflat1=
544 G4RandFlat::shoot((G4double)0.,(G4double)f << 392 CLHEP::RandFlat::shoot((G4double)0.,(G4double)fermiMomentum);
545 G4double ranflat2= << 393 G4double ranflat2=
546 G4RandFlat::shoot((G4double)0.,(G4double)f << 394 CLHEP::RandFlat::shoot((G4double)0.,(G4double)fermiMomentum);
547 G4double ranflat3= << 395 G4double ranflat3=
548 G4RandFlat::shoot((G4double)0.,(G4double)f << 396 CLHEP::RandFlat::shoot((G4double)0.,(G4double)fermiMomentum);
549 G4double ranmax = (ranflat1>ranflat2? ranfla << 397 G4double ranmax = (ranflat1>ranflat2? ranflat1: ranflat2);
550 ranmax = (ranmax>ranflat3? ranmax : ranflat3 << 398 ranmax = (ranmax>ranflat3? ranmax : ranflat3);
551 << 399
552 // Isotropic momentum distribution << 400 // Isotropic momentum distribution
553 G4double costheta = 2.*G4UniformRand() - 1.0 << 401 G4double costheta = 2.*G4UniformRand() - 1.0;
554 G4double sintheta = std::sqrt(1.0 - costheta << 402 G4double sintheta = std::sqrt(1.0 - costheta*costheta);
555 G4double phi = 2.0*pi*G4UniformRand(); << 403 G4double phi = 2.0*pi*G4UniformRand();
556 << 404
557 G4double pz=costheta*ranmax; << 405 G4double pz=costheta*ranmax;
558 G4double px=sintheta*std::cos(phi)*ranmax; << 406 G4double px=sintheta*std::cos(phi)*ranmax;
559 G4double py=sintheta*std::sin(phi)*ranmax; << 407 G4double py=sintheta*std::sin(phi)*ranmax;
560 G4ThreeVector p(px,py,pz); << 408 G4ThreeVector p(px,py,pz);
561 return p; << 409 return p;
562 } << 410 }
563 411
564 << 412 G4ReactionProductVector* G4Nucleus::Fragmentate()
565 G4ReactionProductVector* G4Nucleus::Fragmentat << 413 {
566 { << 414 // needs implementation!
567 // needs implementation! << 415 return NULL;
568 return nullptr; << 416 }
569 } <<
570 417
571 << 418 void G4Nucleus::AddMomentum(const G4ThreeVector aMomentum)
572 void G4Nucleus::AddMomentum(const G4ThreeVecto << 419 {
573 { << 420 momentum+=(aMomentum);
574 momentum+=(aMomentum); << 421 }
575 } <<
576 <<
577 422
578 void G4Nucleus::AddExcitationEnergy( G4double << 423 void G4Nucleus::AddExcitationEnergy( G4double anEnergy )
579 { << 424 {
580 excitationEnergy+=anEnergy; << 425 excitationEnergy+=anEnergy;
581 } << 426 }
582 427
583 /* end of file */ 428 /* end of file */
584 429
585 430