| 1 | /* ======================================================================== *\
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| 2 | !
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| 3 | ! *
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| 4 | ! * This file is part of MARS, the MAGIC Analysis and Reconstruction
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| 5 | ! * Software. It is distributed to you in the hope that it can be a useful
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| 6 | ! * and timesaving tool in analysing Data of imaging Cerenkov telescopes.
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| 7 | ! * It is distributed WITHOUT ANY WARRANTY.
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| 8 | ! *
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| 9 | ! * Permission to use, copy, modify and distribute this software and its
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| 10 | ! * documentation for any purpose is hereby granted without fee,
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| 11 | ! * provided that the above copyright notice appear in all copies and
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| 12 | ! * that both that copyright notice and this permission notice appear
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| 13 | ! * in supporting documentation. It is provided "as is" without express
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| 14 | ! * or implied warranty.
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| 15 | ! *
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| 16 | !
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| 17 | !
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| 18 | ! Author(s): Harald Kornmayer 1/2001 (harald@mppmu.mpg.de)
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| 19 | ! Author(s): Thomas Bretz 12/2000 (tbretz@uni-sw.gwdg.de)
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| 20 | !
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| 21 | ! Copyright: MAGIC Software Development, 2000-2001
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| 22 | !
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| 23 | !
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| 24 | \* ======================================================================== */
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| 25 |
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| 26 | //////////////////////////////////////////////////////////////////////////////
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| 27 | // //
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| 28 | // //
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| 29 | //////////////////////////////////////////////////////////////////////////////
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| 30 | #include "MPhoton.h"
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| 31 |
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| 32 | #include <iostream.h>
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| 33 |
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| 34 | #include <TF1.h>
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| 35 |
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| 36 | ClassImp(MPhoton);
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| 37 |
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| 38 | Double_t MPhoton::Planck(Double_t *x, Double_t *k=NULL)
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| 39 | {
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| 40 | //
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| 41 | // Planck, per unit volume, per unit energy
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| 42 | //
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| 43 | // constants moved out of function, see below
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| 44 | //
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| 45 | Double_t E = x[0]; // [GeV]
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| 46 | Double_t z = k ? k[0] : 0;
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| 47 |
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| 48 | Double_t T = 2.96*(z+1); // [K]
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| 49 | Double_t e = 1.602176462e-19; // [C]
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| 50 | Double_t kB = 1e-9/e*1.3806503e-23; // [GeV/K]
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| 51 |
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| 52 | Double_t EkT = E/kB/T;
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| 53 |
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| 54 | /*
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| 55 | //Double_t c = 299792458; // [m/s]
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| 56 | //Double_t h = 1e-9/e*6.62606876e-34; // [GeVs]
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| 57 | //Double_t hc = h*c; // [GeVm]
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| 58 |
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| 59 | Double_t konst = 4.*TMath::Pi() * 2. / (hc*hc*hc);
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| 60 | return konst * E*E / (exp(EkT)-1.); // [1 / GeV / m^3 ]
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| 61 | */
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| 62 |
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| 63 | return E*E / (exp(EkT)-1.); // [GeV^2]
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| 64 | }
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| 65 |
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| 66 | Double_t MPhoton::Sigma_gg(Double_t *x, Double_t *k=NULL)
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| 67 | {
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| 68 | Double_t s = x[0]; // omega: CM mass
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| 69 |
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| 70 | Double_t E0 = 511e-6; // [GeV]
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| 71 | Double_t r0 = 2.81794092e-15; // [m] = e^2/4/pi/m/eps0/c^2
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| 72 |
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| 73 | Double_t m = E0/s;
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| 74 |
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| 75 | Double_t m2 = m*m;
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| 76 | Double_t beta = sqrt(1.-m2);
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| 77 | Double_t beta2 = 1.-m2;
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| 78 |
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| 79 | Double_t p1 = r0*r0*TMath::Pi()/2;
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| 80 |
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| 81 | // ----- Extreme Relativistic -----
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| 82 | // return p1*2 * m*m*m* (log(2./m)-1);
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| 83 | // --------------------------------
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| 84 |
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| 85 | Double_t p2 = m2;
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| 86 | Double_t p3 = 3.-beta2*beta2;
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| 87 | Double_t p4 = log((1.+beta)/(1.-beta));
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| 88 | Double_t p5 = beta*2*(1.+m2);
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| 89 |
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| 90 | Double_t sigma = p1*p2*(p3*p4-p5); // [m^2]
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| 91 |
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| 92 | return sigma;
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| 93 | }
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| 94 |
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| 95 | Double_t MPhoton::Int1(Double_t *x, Double_t *k=NULL)
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| 96 | {
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| 97 | Double_t costheta = x[0];
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| 98 |
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| 99 | Double_t Eg = k[0];
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| 100 | Double_t Ep = k[1];
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| 101 |
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| 102 | Double_t E0 = 511e-6; // [GeV]
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| 103 |
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| 104 | Double_t s = Eg*Ep/E0*(1.-costheta)*2;
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| 105 |
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| 106 | if (s<E0) // Why is this necessary???
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| 107 | return 0;
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| 108 |
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| 109 | Double_t sigma = Sigma_gg(&s); // [m^2]
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| 110 |
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| 111 | return sigma/2 * (1.-costheta); // [m^2]
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| 112 | }
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| 113 |
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| 114 | Double_t MPhoton::Int2(Double_t *x, Double_t *k)
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| 115 | {
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| 116 | Double_t E0 = 511e-6; // [GeV]
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| 117 |
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| 118 | Double_t Ep = x[0];
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| 119 | Double_t Eg = k[0];
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| 120 |
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| 121 | Double_t z = k[1];
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| 122 |
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| 123 | Double_t val[2] = { Eg, Ep };
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| 124 |
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| 125 | Double_t from = -1.0;
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| 126 | Double_t to = 1.-E0*E0/2./Eg/Ep; // Originally Was: 1.
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| 127 |
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| 128 | TF1 f("int1", Int1, from, to, 2);
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| 129 | Double_t int1 = f.Integral(from, to, val); // [m^2]
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| 130 | Double_t planck = Planck(&Ep, &z); // [GeV^2]
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| 131 |
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| 132 | Double_t res = planck * int1;
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| 133 |
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| 134 | res *= Eg/E0*1e-9; // FIXME!!!!!!!!!! WHICH FACTOR IS THIS????
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| 135 |
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| 136 | return res; // [GeV^2 m^2]
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| 137 | }
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| 138 |
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| 139 | // --------------------------------------------------------------------------
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| 140 | //
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| 141 | // Returns 0 in case IL becomes (numerically) infinite.
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| 142 | //
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| 143 | Double_t MPhoton::InteractionLength(Double_t *x, Double_t *k=NULL)
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| 144 | {
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| 145 | Double_t E0 = 511e-6; // [GeV]
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| 146 | Double_t c = 299792458; // [m/s]
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| 147 | Double_t e = 1.602176462e-19; // [C]
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| 148 | Double_t h = 1e-9/e*6.62606876e-34; // [GeVs]
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| 149 | Double_t hc = h*c; // [GeVm]
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| 150 | Double_t pc = 1./3.258; // [pc/ly]
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| 151 | Double_t ly = 3600.*24.*365.*c; // [m/ly]
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| 152 |
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| 153 | Double_t Eg = x[0];
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| 154 | Double_t z = k ? k[0] : 0;
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| 155 |
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| 156 | Double_t val[2] = { Eg, z };
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| 157 |
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| 158 | Double_t lolim = E0*E0/Eg;
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| 159 | Double_t inf = 4e-12; //E0*E0/Eg * sqrt(Eg);
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| 160 |
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| 161 | TF1 f("int2", Int2, lolim, inf, 2);
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| 162 |
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| 163 | Double_t int2 = f.Integral(lolim, inf, val); //[GeV^3 m^2]
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| 164 |
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| 165 | if (int2==0)
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| 166 | {
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| 167 | //cout << "---> Int2==0 <---" << endl;
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| 168 | return 0;
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| 169 | }
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| 170 |
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| 171 | /* Planck constants: konst */
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| 172 | Double_t konst = 4.*TMath::Pi() * 2. / (hc*hc*hc);
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| 173 | int2 *= konst; // [1 / m]
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| 174 |
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| 175 | Double_t res = 1./ int2; // [m]
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| 176 | res *= pc/ly * 1e-3; // [kpc]
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| 177 |
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| 178 | if (res > 1e50) return 1e50;
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| 179 | if (res < 0) return 1e35;
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| 180 |
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| 181 | return res; //[kpc]
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| 182 | }
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| 183 |
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| 184 | Double_t MPhoton::GetInteractionLength(Double_t energy, Double_t z)
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| 185 | {
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| 186 | return InteractionLength(&energy, &z);
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| 187 | }
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| 188 |
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| 189 | Double_t MPhoton::GetInteractionLength() const
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| 190 | {
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| 191 | return InteractionLength((Double_t*)&fEnergy, (Double_t*)&fZ);
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| 192 | }
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| 193 |
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