Geant4 11.4.0
Toolkit for the simulation of the passage of particles through matter
Loading...
Searching...
No Matches
G4RKG3_Stepper.cc
Go to the documentation of this file.
1//
2// ********************************************************************
3// * License and Disclaimer *
4// * *
5// * The Geant4 software is copyright of the Copyright Holders of *
6// * the Geant4 Collaboration. It is provided under the terms and *
7// * conditions of the Geant4 Software License, included in the file *
8// * LICENSE and available at http://cern.ch/geant4/license . These *
9// * include a list of copyright holders. *
10// * *
11// * Neither the authors of this software system, nor their employing *
12// * institutes,nor the agencies providing financial support for this *
13// * work make any representation or warranty, express or implied, *
14// * regarding this software system or assume any liability for its *
15// * use. Please see the license in the file LICENSE and URL above *
16// * for the full disclaimer and the limitation of liability. *
17// * *
18// * This code implementation is the result of the scientific and *
19// * technical work of the GEANT4 collaboration. *
20// * By using, copying, modifying or distributing the software (or *
21// * any work based on the software) you agree to acknowledge its *
22// * use in resulting scientific publications, and indicate your *
23// * acceptance of all terms of the Geant4 Software license. *
24// ********************************************************************
25//
26// G4RKG3_Stepper implementation
27//
28// Authors: John Apostolakis & Vladimir Grichine (CERN), 30.01.1997
29// -------------------------------------------------------------------
30
31#include "G4RKG3_Stepper.hh"
32#include "G4LineSection.hh"
33#include "G4Mag_EqRhs.hh"
34
39
40void G4RKG3_Stepper::Stepper( const G4double yInput[], // [8]
41 const G4double dydx[], // [6]
42 G4double Step,
43 G4double yOut[], // [8]
44 G4double yErr[] )
45{
46 G4double B[3];
47 G4int nvar = 6 ;
48 G4double by15 = 1. / 15. ; // was 0.066666666 ;
49
50 G4double yTemp[8], dydxTemp[6], yIn[8];
51
52 // Saving yInput because yInput and yOut can be aliases for same array
53 //
54 for(G4int i=0; i<nvar; ++i)
55 {
56 yIn[i]=yInput[i];
57 }
58 yIn[6] = yInput[6];
59 yIn[7] = yInput[7];
60 G4double h = Step * 0.5;
61 hStep = Step;
62 // Do two half steps
63
64 StepNoErr(yIn, dydx,h, yTemp,B) ;
65
66 // Store Bfld for DistChord Calculation
67 //
68 for(auto i=0; i<3; ++i)
69 {
70 BfldIn[i] = B[i];
71 }
72 // RightHandSide(yTemp,dydxTemp) ;
73
74 GetEquationOfMotion()->EvaluateRhsGivenB(yTemp,B,dydxTemp) ;
75 StepNoErr(yTemp,dydxTemp,h,yOut,B);
76
77 // Store midpoint, chord calculation
78
79 fyMidPoint = G4ThreeVector(yTemp[0], yTemp[1], yTemp[2]);
80
81 // Do a full Step
82 //
83 h *= 2 ;
84 StepNoErr(yIn,dydx,h,yTemp,B);
85 for(G4int i=0; i<nvar; ++i)
86 {
87 yErr[i] = yOut[i] - yTemp[i] ;
88 yOut[i] += yErr[i]*by15 ; // Provides 5th order of accuracy
89 }
90
91 // Store values for DistChord method
92 //
93 fyInitial = G4ThreeVector( yIn[0], yIn[1], yIn[2]);
94 fpInitial = G4ThreeVector( yIn[3], yIn[4], yIn[5]);
95 fyFinal = G4ThreeVector( yOut[0], yOut[1], yOut[2]);
96}
97
98// ---------------------------------------------------------------------------
99
100// Integrator for RK from G3 with evaluation of error in solution and delta
101// geometry based on naive similarity with the case of uniform magnetic field.
102// B1[3] is input and is the first magnetic field values
103// B2[3] is output and is the final magnetic field values.
104//
106 const G4double*,
107 G4double,
108 G4double*,
109 G4double&,
110 G4double&,
111 const G4double*,
112 G4double* )
113
114{
115 G4Exception("G4RKG3_Stepper::StepWithEst()", "GeomField0001",
116 FatalException, "Method no longer used.");
117}
118
119// -----------------------------------------------------------------
120
121// Integrator RK Stepper from G3 with only two field evaluation per Step.
122// It is used in propagation initial Step by small substeps after solution
123// error and delta geometry considerations. B[3] is magnetic field which
124// is passed from substep to substep.
125//
127 const G4double dydx[6],
128 G4double Step,
129 G4double tOut[8],
130 G4double B[3] )
131
132{
133
134 // Copy and edit the routine above, to delete alpha2, beta2, ...
135 //
136 G4double K1[7], K2[7], K3[7], K4[7];
137 G4double tTemp[8]={0.0}, yderiv[6]={0.0};
138
139 // Need Momentum value to give correct values to the coefficients in
140 // equation. Integration on unit velocity, but tIn[3,4,5] is momentum
141
142 G4double mom, inverse_mom;
143 const G4double c1=0.5, c2=0.125, c3=1./6.;
144
145 // Correction for momentum not a velocity
146 // Need the protection !!! must be not zero
147 //
148 mom = std::sqrt(tIn[3]*tIn[3]+tIn[4]*tIn[4]+tIn[5]*tIn[5]);
149 inverse_mom = 1./mom;
150 for(auto i=0; i<3; ++i)
151 {
152 K1[i] = Step * dydx[i+3]*inverse_mom;
153 tTemp[i] = tIn[i] + Step*(c1*tIn[i+3]*inverse_mom + c2*K1[i]) ;
154 tTemp[i+3] = tIn[i+3] + c1*K1[i]*mom ;
155 }
156
157 GetEquationOfMotion()->EvaluateRhsReturnB(tTemp,yderiv,B) ;
158
159 for(auto i=0; i<3; ++i)
160 {
161 K2[i] = Step * yderiv[i+3]*inverse_mom;
162 tTemp[i+3] = tIn[i+3] + c1*K2[i]*mom ;
163 }
164
165 // Given B, calculate yderiv !
166 //
167 GetEquationOfMotion()->EvaluateRhsGivenB(tTemp,B,yderiv) ;
168
169 for(auto i=0; i<3; ++i)
170 {
171 K3[i] = Step * yderiv[i+3]*inverse_mom;
172 tTemp[i] = tIn[i] + Step*(tIn[i+3]*inverse_mom + c1*K3[i]) ;
173 tTemp[i+3] = tIn[i+3] + K3[i]*mom ;
174 }
175
176 // Calculates y-deriv(atives) & returns B too!
177 //
178 GetEquationOfMotion()->EvaluateRhsReturnB(tTemp,yderiv,B) ;
179
180 for(auto i=0; i<3; ++i) // Output trajectory vector
181 {
182 K4[i] = Step * yderiv[i+3]*inverse_mom;
183 tOut[i] = tIn[i] + Step*(tIn[i+3]*inverse_mom+ (K1[i]+K2[i]+K3[i])*c3) ;
184 tOut[i+3] = tIn[i+3] + mom*(K1[i] + 2*K2[i] + 2*K3[i] +K4[i])*c3 ;
185 }
186 tOut[6] = tIn[6];
187 tOut[7] = tIn[7];
188}
189
190// ---------------------------------------------------------------------------
191
193{
194 // Soon: must check whether h/R > 2 pi !!
195 // Method below is good only for < 2 pi
196
197 G4double distChord,distLine;
198
199 if (fyInitial != fyFinal)
200 {
201 distLine = G4LineSection::Distline(fyMidPoint,fyInitial,fyFinal);
202 distChord = distLine;
203 }
204 else
205 {
206 distChord = (fyMidPoint-fyInitial).mag();
207 }
208
209 return distChord;
210}
G4double B(G4double temperature)
@ FatalException
void G4Exception(const char *originOfException, const char *exceptionCode, G4ExceptionSeverity severity, const char *description)
CLHEP::Hep3Vector G4ThreeVector
double G4double
Definition G4Types.hh:83
int G4int
Definition G4Types.hh:85
virtual void EvaluateRhsGivenB(const G4double y[], const G4double B[3], G4double dydx[]) const =0
void EvaluateRhsReturnB(const G4double y[], G4double dydx[], G4double Field[]) const
static G4double Distline(const G4ThreeVector &OtherPnt, const G4ThreeVector &LinePntA, const G4ThreeVector &LinePntB)
G4MagIntegratorStepper(G4EquationOfMotion *Equation, G4int numIntegrationVariables, G4int numStateVariables=12, G4bool isFSAL=false)
G4EquationOfMotion * GetEquationOfMotion()
G4Mag_EqRhs is the "standard" equation of motion of a particle in a pure magnetic field.
G4double DistChord() const override
void StepWithEst(const G4double tIn[8], const G4double dydx[6], G4double Step, G4double tOut[8], G4double &alpha2, G4double &beta2, const G4double B1[3], G4double B2[3])
void Stepper(const G4double yIn[], const G4double dydx[], G4double h, G4double yOut[], G4double yErr[]) override
void StepNoErr(const G4double tIn[8], const G4double dydx[6], G4double Step, G4double tOut[8], G4double B[3])
G4RKG3_Stepper(G4Mag_EqRhs *EqRhs)