// // ******************************************************************** // * License and Disclaimer * // * * // * The Geant4 software is copyright of the Copyright Holders of * // * the Geant4 Collaboration. It is provided under the terms and * // * conditions of the Geant4 Software License, included in the file * // * LICENSE and available at http://cern.ch/geant4/license . These * // * include a list of copyright holders. * // * * // * Neither the authors of this software system, nor their employing * // * institutes,nor the agencies providing financial support for this * // * work make any representation or warranty, express or implied, * // * 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 * // * use in resulting scientific publications, and indicate your * // * acceptance of all terms of the Geant4 Software license. * // ******************************************************************** // /// \file MuCrossSections.cc /// \brief Implementation of the MuCrossSections class #include "MuCrossSections.hh" #include "G4DataVector.hh" #include "G4Exp.hh" #include "G4Log.hh" #include "G4Material.hh" #include "G4MuonMinus.hh" #include "G4NistManager.hh" #include "G4PhysicalConstants.hh" #include "G4SystemOfUnits.hh" //....oooOO0OOooo........oooOO0OOooo........oooOO0OOooo........oooOO0OOooo...... using namespace std; MuCrossSections::MuCrossSections() { fNist = G4NistManager::Instance(); fMuonMass = G4MuonMinus::MuonMinus()->GetPDGMass(); fMueRatio = fMuonMass / CLHEP::electron_mass_c2; } //....oooOO0OOooo........oooOO0OOooo........oooOO0OOooo........oooOO0OOooo...... G4double MuCrossSections::CR_Macroscopic(const G4String& process, const G4Material* material, G4double tkin, G4double ep) // return the macroscopic cross section (1/L) in GEANT4 internal units { const G4ElementVector* theElementVector = material->GetElementVector(); const G4double* NbOfAtomsPerVolume = material->GetVecNbOfAtomsPerVolume(); G4double SIGMA = 0.; G4int nelm = material->GetNumberOfElements(); for (G4int i = 0; i < nelm; ++i) { const G4Element* element = (*theElementVector)[i]; SIGMA += NbOfAtomsPerVolume[i] * CR_PerAtom(process, element, tkin, ep); } return SIGMA; } //....oooOO0OOooo........oooOO0OOooo........oooOO0OOooo........oooOO0OOooo...... G4double MuCrossSections::CR_PerAtom(const G4String& process, const G4Element* element, G4double tkin, G4double ep) { G4double z = element->GetZ(); G4double a = element->GetA(); G4double sigma = 0.; if (process == "muBrems") sigma = CRB_Mephi(z, a / (g / mole), tkin / GeV, ep / GeV) * (cm2 / (g * GeV)) * a / Avogadro; else if (process == "muIoni") sigma = CRK_Mephi(z, a / (g / mole), tkin / GeV, ep / GeV) * (cm2 / (g * GeV)) * a / Avogadro; // else if (process == "muNucl") else if (process == "muonNuclear") sigma = CRN_Mephi(z, a / (g / mole), tkin / GeV, ep / GeV) * (cm2 / (g * GeV)) * a / Avogadro; else if (process == "muPairProd") sigma = CRP_Mephi(z, a / (g / mole), tkin / GeV, ep / GeV) * (cm2 / (g * GeV)) * a / Avogadro; else if (process == "muToMuonPairProd") sigma = CRM_Mephi(z, tkin, ep); return sigma; } //....oooOO0OOooo........oooOO0OOooo........oooOO0OOooo........oooOO0OOooo...... G4double MuCrossSections::CRB_Mephi(G4double z, G4double a, G4double tkin, G4double ep) //*********************************************************************** //*** crb_g4_1.inc in comparison with crb_.inc, following //*** changes are introduced (September 24th, 1998): //*** 1) function crb_g4 (Z,A,Tkin,EP), Tkin is kinetic energy //*** 2) special case of hidrogen (Z<1.5; b,b1,Dn_star) //*** Numerical comparison: 5 decimal digits coincide. //*** //*** Cross section for bremsstrahlung by fast muon //*** By R.P.Kokoulin, September 1998 //*** Formulae from Kelner,Kokoulin,Petrukhin 1995, Preprint MEPhI //*** (7,18,19,20,21,25,26); Dn (18) is modified to incorporate //*** Bugaev's inelatic nuclear correction (28) for Z > 1. //*********************************************************************** { // G4double Z,A,Tkin,EP; G4double crb_g4; G4double e, v, delta, rab0, z_13, dn, b, b1, dn_star, rab1, fn, epmax1, fe, rab2; // G4double ame = 0.51099907e-3; // GeV G4double lamu = 0.105658389; // GeV G4double re = 2.81794092e-13; // cm G4double avno = 6.022137e23; G4double alpha = 1. / 137.036; G4double rmass = lamu / ame; // "207" G4double coeff = 16. / 3. * alpha * avno * (re / rmass) * (re / rmass); // cm^2 G4double sqrte = 1.64872127; // sqrt(2.71828...) G4double btf = 183.; G4double btf1 = 1429.; G4double bh = 202.4; G4double bh1 = 446.; //*** if (ep >= tkin) { return 0.; } e = tkin + lamu; v = ep / e; delta = lamu * lamu * v / (2. * (e - ep)); // qmin rab0 = delta * sqrte; G4int Z = G4lrint(z); z_13 = 1. / fNist->GetZ13(z); // //*** nuclear size and excitation, screening parameters dn = 1.54 * fNist->GetA27(Z); if (z <= 1.5) // special case for hydrogen { b = bh; b1 = bh1; dn_star = dn; } else { b = btf; b1 = btf1; dn_star = pow(dn, (1. - 1. / z)); // with Bugaev's correction } //*** nucleus contribution logarithm rab1 = b * z_13; fn = G4Log(rab1 / (dn_star * (ame + rab0 * rab1)) * (lamu + delta * (dn_star * sqrte - 2.))); if (fn < 0.) fn = 0.; //*** electron contribution logarithm epmax1 = e / (1. + lamu * rmass / (2. * e)); if (ep >= epmax1) { fe = 0.; } else { rab2 = b1 * z_13 * z_13; fe = G4Log(rab2 * lamu / ((1. + delta * rmass / (ame * sqrte)) * (ame + rab0 * rab2))); if (fe < 0.) fe = 0.; } crb_g4 = coeff * (1. - v * (1. - 0.75 * v)) * z * (z * fn + fe) / (a * ep); return crb_g4; } //....oooOO0OOooo........oooOO0OOooo........oooOO0OOooo........oooOO0OOooo...... G4double MuCrossSections::CRK_Mephi(G4double z, G4double a, G4double tkin, G4double ep) //*********************************************************************** //*** Cross section for knock-on electron production by fast muons //*** (including bremsstrahlung e-diagrams and rad. correction). //*** Units: cm^2/(g*GeV); Tkin, ep - GeV. //*** By R.P.Kokoulin, October 1998 //*** Formulae from Kelner,Kokoulin,Petrukhin, Phys.Atom.Nuclei, 1997 //*** (a bit simplified Kelner's version of Eq.30 - with 2 logarithms). //*** { // G4double Z,A,Tkin,EP; G4double crk_g4; G4double v, sigma0, a1, a3; // G4double ame = 0.51099907e-3; // GeV G4double lamu = 0.105658389; // GeV G4double re = 2.81794092e-13; // cm G4double avno = 6.022137e23; G4double alpha = 1. / 137.036; G4double lpi = 3.141592654; G4double bmu = lamu * lamu / (2. * ame); G4double coeff0 = avno * 2. * lpi * ame * re * re; G4double coeff1 = alpha / (2. * lpi); //*** G4double e = tkin + lamu; G4double epmax = e / (1. + bmu / e); if (ep >= epmax) { return 0.0; } v = ep / e; sigma0 = coeff0 * (z / a) * (1. - ep / epmax + 0.5 * v * v) / (ep * ep); a1 = G4Log(1. + 2. * ep / ame); a3 = G4Log(4. * e * (e - ep) / (lamu * lamu)); crk_g4 = sigma0 * (1. + coeff1 * a1 * (a3 - a1)); return crk_g4; } //....oooOO0OOooo........oooOO0OOooo........oooOO0OOooo........oooOO0OOooo...... G4double MuCrossSections::CRN_Mephi(G4double, G4double a, G4double tkin, G4double ep) //*********************************************************************** //*** Differential cross section for photonuclear muon interaction. //*** Formulae from Borog & Petrukhin, 1975 //*** Real photon cross section: Caldwell e.a., 1979 //*** Nuclear shadowing: Brodsky e.a., 1972 //*** Units: cm^2 / g GeV. //*** CRN_G4_1.inc January 31st, 1998 R.P.Kokoulin //*********************************************************************** { // G4double Z,A,Tkin,EP; G4double crn_g4; G4double e, aeff, sigph, v, v1, v2, amu2, up, down; //*** G4double lamu = 0.105658389; // GeV G4double avno = 6.022137e23; G4double amp = 0.9382723; // GeV G4double lpi = 3.14159265; G4double alpha = 1. / 137.036; //*** G4double epmin_phn = 0.20; // GeV G4double alam2 = 0.400000; // GeV**2 G4double alam = 0.632456; // sqrt(alam2) G4double coeffn = alpha / lpi * avno * 1e-30; // cm^2/microbarn //*** e = tkin + lamu; crn_g4 = 0.; if (ep >= e - 0.5 * amp || ep <= epmin_phn) return crn_g4; aeff = 0.22 * a + 0.78 * pow(a, 0.89); // shadowing sigph = 49.2 + 11.1 * G4Log(ep) + 151.8 / std::sqrt(ep); // microbarn v = ep / e; v1 = 1. - v; v2 = v * v; amu2 = lamu * lamu; up = e * e * v1 / amu2 * (1. + amu2 * v2 / (alam2 * v1)); down = 1. + ep / alam * (1. + alam / (2. * amp) + ep / alam); crn_g4 = coeffn * aeff / a * sigph / ep * (-v1 + (v1 + 0.5 * v2 * (1. + 2. * amu2 / alam2)) * log(up / down)); if (crn_g4 < 0.) crn_g4 = 0.; return crn_g4; } //....oooOO0OOooo........oooOO0OOooo........oooOO0OOooo........oooOO0OOooo...... G4double MuCrossSections::CRP_Mephi(G4double z, G4double a, G4double tkin, G4double ep) //********************************************************************** //*** crp_g4_1.inc in comparison with crp_m.inc, following //*** changes are introduced (January 16th, 1998): //*** 1) Avno/A, cm^2/gram GeV //*** 2) zeta_loss(E,Z) from Kelner 1997, Eqs.(53-54) //*** 3) function crp_g4 (Z,A,Tkin,EP), Tkin is kinetic energy //*** 4) bbb=183 (Thomas-Fermi) //*** 5) special case of hidrogen (Z<1.5), bbb,g1,g2 //*** 6) expansions in 'xi' are simplified (Jan.17th,1998) //*** //*** Cross section for electron pair production by fast muon //*** By R.P.Kokoulin, December 1997 //*** Formulae from Kokoulin & Petrukhin 1971, Hobart, Eqs.(1,8,9,10) { // G4double Z,A,Tkin,EP; G4double crp_g4; G4double bbbtf, bbbh, g1tf, g2tf, g1h, g2h, e, z13, e1, alf, a3, bbb; G4double g1, g2, zeta1, zeta2, zeta, z2, screen0, a0, a1, bet, xi0, del; G4double tmn, sum, a4, a5, a6, a7, a9, xi, xii, xi1, screen, yeu, yed, ye1; G4double ale, cre, be, fe, ymu, ymd, ym1, alm_crm, a10, bm, fm; // G4double ame = 0.51099907e-3; // GeV G4double lamu = 0.105658389; // GeV G4double re = 2.81794092e-13; // cm G4double avno = 6.022137e23; G4double lpi = 3.14159265; G4double alpha = 1. / 137.036; G4double rmass = lamu / ame; // "207" G4double coeff = 4. / (3. * lpi) * (alpha * re) * (alpha * re) * avno; // cm^2 G4double sqrte = 1.64872127; // sqrt(2.71828...) G4double c3 = 3. * sqrte * lamu / 4.; // for limits G4double c7 = 4. * ame; // -"- G4double c8 = 6. * lamu * lamu; // -"- G4double xgi[8] = {.0199, .1017, .2372, .4083, .5917, .7628, .8983, .9801}; // Gauss, 8 G4double wgi[8] = {.0506, .1112, .1569, .1813, .1813, .1569, .1112, .0506}; // Gauss, 8 bbbtf = 183.; // for the moment... bbbh = 202.4; // for the moment... g1tf = 1.95e-5; g2tf = 5.3e-5; g1h = 4.4e-5; g2h = 4.8e-5; e = tkin + lamu; z13 = fNist->GetZ13(G4lrint(z)); e1 = e - ep; crp_g4 = 0.; if (e1 <= c3 * z13) return crp_g4; // ep > max alf = c7 / ep; // 4m/ep a3 = 1. - alf; if (a3 <= 0.) return crp_g4; // ep < min //*** zeta calculation if (z <= 1.5) // special case of hidrogen { bbb = bbbh; g1 = g1h; g2 = g2h; } else { bbb = bbbtf; g1 = g1tf; g2 = g2tf; } zeta1 = 0.073 * G4Log(e / (lamu + g1 * z13 * z13 * e)) - 0.26; if (zeta1 > 0.) { zeta2 = 0.058 * log(e / (lamu + g2 * z13 * e)) - 0.14; zeta = zeta1 / zeta2; } else { zeta = 0.; } z2 = z * (z + zeta); // //*** just to check (for comparison with crp_m) // z2=z*(z+1.) // bbb=189. //*** screen0 = 2. * ame * sqrte * bbb / (z13 * ep); // be careful with "ame" a0 = e * e1; a1 = ep * ep / a0; // 2*beta bet = 0.5 * a1; // beta xi0 = 0.25 * rmass * rmass * a1; // xi0 del = c8 / a0; // 6mu^2/EE' tmn = G4Log((alf + 2. * del * a3) / (1. + (1. - del) * sqrt(a3))); // log(1-rmax) sum = 0.; for (G4int i = 0; i < 8; ++i) { a4 = G4Exp(tmn * xgi[i]); // 1-r a5 = a4 * (2. - a4); // 1-r2 a6 = 1. - a5; // r2 a7 = 1. + a6; // 1+r2 a9 = 3. + a6; // 3+r2 xi = xi0 * a5; xii = 1. / xi; xi1 = 1. + xi; screen = screen0 * xi1 / a5; yeu = 5. - a6 + 4. * bet * a7; yed = 2. * (1. + 3. * bet) * G4Log(3. + xii) - a6 - a1 * (2. - a6); ye1 = 1. + yeu / yed; ale = G4Log(bbb / z13 * std::sqrt(xi1 * ye1) / (1. + screen * ye1)); cre = 0.5 * G4Log(1. + (1.5 / rmass * z13) * (1.5 / rmass * z13) * xi1 * ye1); if (xi <= 1e3) { be = ((2. + a6) * (1. + bet) + xi * a9) * G4Log(1. + xii) + (a5 - bet) / xi1 - a9; } else { be = (3. - a6 + a1 * a7) / (2. * xi); // -(6.-5.*a6+3.*bet*a6)/(6.*xi*xi); } fe = std::max(0., (ale - cre) * be); ymu = 4. + a6 + 3. * bet * a7; ymd = a7 * (1.5 + a1) * G4Log(3. + xi) + 1. - 1.5 * a6; ym1 = 1. + ymu / ymd; alm_crm = G4Log(bbb * rmass / (1.5 * z13 * z13 * (1. + screen * ym1))); if (xi >= 1e-3) { a10 = (1. + a1) * a5; // (1+2b)(1-r2) bm = (a7 * (1. + 1.5 * bet) - a10 * xii) * G4Log(xi1) + xi * (a5 - bet) / xi1 + a10; } else { bm = (5. - a6 + bet * a9) * (xi / 2.); // -(11.-5.*a6+.5*bet*(5.+a6))*(xi*xi/6.) } fm = max(0., (alm_crm)*bm); //*** sum = sum + a4 * (fe + fm / (rmass * rmass)) * wgi[i]; } crp_g4 = -tmn * sum * (z2 / a) * coeff * e1 / (e * ep); return crp_g4; } //....oooOO0OOooo........oooOO0OOooo........oooOO0OOooo........oooOO0OOooo...... G4double MuCrossSections::CRM_Mephi(G4double Z, G4double tkin, G4double pairEnergy) { /* ||Cross section for pair production of muons by fast muon ||By Siddharth Yajaman 19-07-2022 ||Based on the formulae from Kelner, Kokoulin and Petrukhin, ||Physics of Atomic Nuclei, Vol. 63, No. 9, 2000, pp. 1603-1611 ||Equations (15) - (22) */ const G4double xgi[] = {0.0198550717512320, 0.1016667612931865, 0.2372337950418355, 0.4082826787521750, 0.5917173212478250, 0.7627662049581645, 0.8983332387068135, 0.9801449282487680}; const G4double wgi[] = {0.0506142681451880, 0.1111905172266870, 0.1568533229389435, 0.1813418916891810, 0.1813418916891810, 0.1568533229389435, 0.1111905172266870, 0.0506142681451880}; static const G4double factorForCross = 2. / (3 * CLHEP::pi) * pow(CLHEP::fine_structure_const * CLHEP::classic_electr_radius / fMueRatio, 2); if (pairEnergy <= 2. * fMuonMass) return 0.0; G4double totalEnergy = tkin + fMuonMass; G4double residEnergy = totalEnergy - pairEnergy; if (residEnergy <= fMuonMass) return 0.0; G4double a0 = 1.0 / (totalEnergy * residEnergy); G4double rhomax = 1.0 - 2 * fMuonMass / pairEnergy; G4double tmnexp = 1. - rhomax; if (tmnexp >= 1.0) { return 0.0; } G4double tmn = G4Log(tmnexp); G4double z2 = Z * Z; G4double beta = 0.5 * pairEnergy * pairEnergy * a0; G4double xi0 = 0.5 * beta; // Gaussian integration in ln(1-ro) ( with 8 points) G4double rho[8]; G4double rho2[8]; G4double xi[8]; G4double xi1[8]; G4double xii[8]; for (G4int i = 0; i < 8; ++i) { rho[i] = G4Exp(tmn * xgi[i]) - 1.0; // rho = -asymmetry rho2[i] = rho[i] * rho[i]; xi[i] = xi0 * (1.0 - rho2[i]); xi1[i] = 1.0 + xi[i]; xii[i] = 1.0 / xi[i]; } G4double ximax = xi0 * (1. - rhomax * rhomax); G4double Y = 10 * sqrt(fMuonMass / totalEnergy); G4double U[8]; for (G4int i = 0; i < 8; ++i) { U[i] = U_func(Z, rho2[i], xi[i], Y, pairEnergy); } G4double UMax = U_func(Z, rhomax * rhomax, ximax, Y, pairEnergy); G4double sum = 0.0; for (G4int i = 0; i < 8; ++i) { G4double X = 1 + U[i] - UMax; G4double lnX = G4Log(X); G4double phi = ((2 + rho2[i]) * (1 + beta) + xi[i] * (3 + rho2[i])) * G4Log(1 + xii[i]) - 1 - 3 * rho2[i] + beta * (1 - 2 * rho2[i]) + ((1 + rho2[i]) * (1 + 1.5 * beta) - xii[i] * (1 + 2 * beta) * (1 - rho2[i])) * G4Log(xi1[i]); sum += wgi[i] * (1.0 + rho[i]) * phi * lnX; } return -tmn * sum * factorForCross * z2 * residEnergy / (totalEnergy * pairEnergy); } //....oooOO0OOooo........oooOO0OOooo........oooOO0OOooo........oooOO0OOooo...... G4double MuCrossSections::U_func(G4double Z, G4double rho2, G4double xi, G4double Y, G4double pairEnergy, const G4double B) { G4int z = G4lrint(Z); G4double A27 = fNist->GetA27(z); G4double Z13 = fNist->GetZ13(z); static const G4double sqe = 2 * std::sqrt(G4Exp(1.0)) * fMuonMass * fMuonMass; G4double res = (0.65 * B / (A27 * Z13) * fMueRatio) / (1 + (sqe * B * (1 + xi) * (1 + Y)) / (Z13 * CLHEP::electron_mass_c2 * pairEnergy * (1 - rho2))); return res; } //....oooOO0OOooo........oooOO0OOooo........oooOO0OOooo........oooOO0OOooo......