G4KalbachCrossSection.cc

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// V.Ivanchenko 26.02.2018
// 
 
#include "G4KalbachCrossSection.hh"
#include "G4Exp.hh"
#include "G4Pow.hh"
 
//from subroutine sigpar of PRECO-2000  by Constance Kalbach Walker
//     Calculate optical model reaction cross sections
//     using the empirical parameterization
//     of Narasimha Murthy, Chaterjee, and Gupta
//     going over to the geometrical limit at high energy.
//
//           Proton cross sections scaled down with signor for a<100
//           (appropriate for becchetti-greenlees potential).
//           p2 reduced and global red'n factor introduced below Bc
//           Neutron cross sections scaled down with signor for a<40
//           Scaled up for A>210 (added June '98 to conform with
//           my published papers)
//           (appropriate for Mani et al potential)
//
 
// index: 0-neutron, 1-proton, 2-deuteron, 3-triton, 4-He3, 5-He4
// parameters: p0, p1, p2, lambda0, lambda1, mu0, mu1, nu0, nu1, nu2, ra
 
static const G4double paramK[6][11] = {
  // n from mani, melkanoff and iori
  {-312., 0.,      0.,  12.10,  -11.27, 234.1, 38.26, 1.55,  -106.1, 1280.8, 0.0},
  // p from  becchetti and greenlees (but modified with sub-barrier
  // correction function and p2 changed from -449)
  {15.72, 9.65, -300.,  0.00437,-16.58, 244.7, 0.503, 273.1, -182.4, -1.872, 0.0},
  // d from o.m. of perey and perey
  {0.798, 420.3,-1651., 0.00619, -7.54, 583.5, 0.337, 421.8, -474.5, -3.592, 0.8},
  // t from o.m. of hafele, flynn et al
  {-21.45,484.7,-1608., 0.0186, -8.9,   686.3, 0.325, 368.9, -522.2, -4.998, 0.8},
  // 3he from o.m. of gibson et al
  {-2.88,205.6, -1487.,0.00459,-8.93,   611.2, 0.35 , 473.8, -468.2, -2.225, 0.8},
  // alpha from huizenga and igo 
  { 10.95,-85.2, 1146.,  0.0643,-13.96, 781.2,  0.29, -304.7,-470.0, -8.580, 1.2}
};
 
G4double G4KalbachCrossSection::ComputePowerParameter(G4int resA, G4int idx)
{
  return G4Pow::GetInstance()->powZ(resA, paramK[idx][6]);
}
 
G4double 
G4KalbachCrossSection::ComputeCrossSection(G4double K, G4double cb,  
                           G4double resA13, G4double amu1, 
                           G4int idx, G4int Z, G4int A, 
                           G4int resA)
{
  G4double sig = 0.0;
  G4double signor = 1.0; 
  G4double lambda, mu, nu;
  G4double ec = 0.5;
  if(0 < Z) { ec = cb; }
  //JMQ 13.02.2009 tuning for improving cluster emission ddxs 
  //               (spallation benchmark) 
  /*
    G4double xx = 1.7;
    if(1 == A) { xx = 1.5; }
    ec = 1.44 * Z * resZ / (xx*resA13 + paramK[idx][10]);
    }
  */
  G4double ecsq = ec*ec;
  G4double elab = K * (A + resA) / G4double(resA);    
    
  if(idx == 0) { // parameterization for neutron
 
    if(resA < 40)       { signor =0.7 + resA*0.0075; }
    else if(resA > 210) { signor = 1. + (resA-210)*0.004; }
    lambda = paramK[idx][3]/resA13 + paramK[idx][4];
    mu = (paramK[idx][5] + paramK[idx][6]*resA13)*resA13;
    // JMQ 20.11.2008 very low energy behaviour corrected 
    //                (problem for A (apprx.)>60) fix for avoiding  
    //                neutron xs going to zero at very low energies
    nu = std::abs((paramK[idx][7]*resA + paramK[idx][8]*resA13)*resA13 
          + paramK[idx][9]);
 
  } else { // parameterization for charged 
    // proton correction
    if(idx == 1) {
      if (resA <= 60)      { signor = 0.92; }
      else if (resA < 100) { signor = 0.8 + resA*0.002; }
    }
    lambda = paramK[idx][3]*resA + paramK[idx][4];
    mu = paramK[idx][5]*amu1;
    nu = amu1* (paramK[idx][7] + paramK[idx][8]*ec + paramK[idx][9]*ecsq);
  }
  /*
    G4cout << "## idx= " << idx << " K= " << K << " elab= " << elab << "  ec= " << ec 
    << " lambda= " << lambda << " mu= " << mu << "  nu= " << nu << G4endl; 
  */
  // threashold cross section
  if(elab < ec) {
    G4double p = paramK[idx][0];
    if(0 < Z) { p += paramK[idx][1]/ec + paramK[idx][2]/ecsq; }
    G4double a = -2*p*ec + lambda - nu/ecsq;
    G4double b = p*ecsq + mu + 2*nu/ec;
    G4double ecut;
    G4double det = a*a - 4*p*b;
    if (det > 0.0) { ecut = (std::sqrt(det) - a)/(2*p); }
    else           { ecut = -a/(2*p); }
 
    //G4cout << "  elab= " << elab << " ecut= " << ecut << " sig= " << sig
    //       << "  sig1= " << (p*elab*elab + a*elab + b)*signor << G4endl;
    // If ecut>0, sig=0 at elab=ecut
    if(0 == idx) {
      sig = (lambda*ec + mu + nu/ec)*signor*std::sqrt(elab/ec);
    } else if(elab >= ecut) { 
      sig = (p*elab*elab + a*elab + b)*signor; 
 
      // extra proton correction
      if(1 == idx) {
    // c and w are for global correction factor for 
    // they are scaled down for light targets where ec is low.
    G4double cc = std::min(3.15, ec*0.5);
    G4double signor2 = (ec - elab - cc) *3.15/ (0.7*cc);
    sig /= (1. + G4Exp(signor2));
      }
    }
    //G4cout << "       ecut= " << ecut << " a= " << a << "  b= " << b 
    //     <<  " signor= " << signor << " sig= " << sig << G4endl;  
 
    // high energy cross section
  } else {
    // etest is the energy above which the rxn cross section is
    // compared with the geometrical limit and the max taken.
 
    // neutron parameters
    G4double etest  = 32.;
    G4double xnulam = 1.0;
 
    // parameters for charged
    static const G4double flow = 1.e-18;
    static const G4double spill= 1.e+18;
    if(0 < Z) {
      etest = 0.0;
      xnulam = nu / lambda;
      xnulam = std::min(xnulam, spill); 
      if (xnulam >= flow) { 
    if(1 == idx) { etest = std::sqrt(xnulam) + 7.; }
    else         { etest = 1.2 *std::sqrt(xnulam); }
      }
    }
    // ** For xnulam.gt.0, sig reaches a maximum at sqrt(xnulam).
    sig = (lambda*elab + mu + nu/elab)*signor;
    if (xnulam >= flow && elab >= etest) {
      G4double geom = std::sqrt(A*K);
      geom = 1.23*resA13 + paramK[idx][10] + 4.573/geom;
      geom = 31.416 * geom * geom;
      sig = std::max(sig, geom);
    }
  }
  sig = std::max(sig, 0.0);
  //G4cout << "  ---- sig= " << sig << G4endl;
  return sig;
}