1 | SUBROUTINE MUBREM
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2 |
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3 | C-----------------------------------------------------------------------
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4 | C MU(ON) BREM(SSTRAHLUNG)
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5 | C
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6 | C TREATES MUON BREMSSTRAHLUNG (WITHOUT POLARISATION EFFECTS)
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7 | C IN ANALOGY WITH SUBROUTINE GBREMM FROM GEANT WRITTEN BY L. URBAN
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8 | C EXPLANATIONS SEE CERN PROGRM LIBRARY LONG WRITEUP W5013
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9 | C THIS SUBROUTINE IS CALLED FROM MUTRAC
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10 | C
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11 | C DESIGN : D. HECK IK3 FZK KARLSRUHE
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12 | C-----------------------------------------------------------------------
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13 |
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14 | IMPLICIT NONE
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15 | *KEEP,CONST.
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16 | COMMON /CONST/ PI,PI2,OB3,TB3,ENEPER
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17 | DOUBLE PRECISION PI,PI2,OB3,TB3,ENEPER
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18 | *KEEP,ELABCT.
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19 | COMMON /ELABCT/ ELCUT
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20 | DOUBLE PRECISION ELCUT(4)
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21 | *KEEP,GENER.
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22 | COMMON /GENER/ GEN,ALEVEL
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23 | DOUBLE PRECISION GEN,ALEVEL
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24 | *KEEP,MUPART.
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25 | COMMON /MUPART/ AMUPAR,BCUT,CMUON,FMUBRM,FMUORG
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26 | DOUBLE PRECISION AMUPAR(14),BCUT,CMUON(11)
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27 | LOGICAL FMUBRM,FMUORG
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28 | *KEEP,PAM.
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29 | COMMON /PAM/ PAMA,SIGNUM
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30 | DOUBLE PRECISION PAMA(6000),SIGNUM(6000)
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31 | *KEEP,PARPAR.
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32 | COMMON /PARPAR/ CURPAR,SECPAR,PRMPAR,OUTPAR,C,
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33 | * E00,E00PN,PTOT0,PTOT0N,THICKH,ITYPE,LEVL
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34 | DOUBLE PRECISION CURPAR(14),SECPAR(14),PRMPAR(14),OUTPAR(14),
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35 | * C(50),E00,E00PN,PTOT0,PTOT0N,THICKH
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36 | INTEGER ITYPE,LEVL
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37 | *KEEP,PARPAE.
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38 | DOUBLE PRECISION GAMMA,COSTHE,PHI,H,T,X,Y,CHI,BETA,GCM,ECM
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39 | EQUIVALENCE (CURPAR(2),GAMMA), (CURPAR(3),COSTHE),
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40 | * (CURPAR(4), PHI ), (CURPAR(5), H ),
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41 | * (CURPAR(6), T ), (CURPAR(7), X ),
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42 | * (CURPAR(8), Y ), (CURPAR(9), CHI ),
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43 | * (CURPAR(10),BETA), (CURPAR(11),GCM ),
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44 | * (CURPAR(12),ECM )
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45 | *KEEP,POLAR.
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46 | COMMON /POLAR/ POLART,POLARF
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47 | DOUBLE PRECISION POLART,POLARF
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48 | *KEEP,RANDPA.
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49 | COMMON /RANDPA/ FAC,U1,U2,RD,NSEQ,ISEED,KNOR
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50 | DOUBLE PRECISION FAC,U1,U2
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51 | REAL RD(3000)
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52 | INTEGER ISEED(103,10),NSEQ
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53 | LOGICAL KNOR
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54 | *KEEP,REST.
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55 | COMMON /REST/ CONTNE,TAR,LT
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56 | DOUBLE PRECISION CONTNE(3),TAR
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57 | INTEGER LT
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58 | *KEEP,RUNPAR.
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59 | COMMON /RUNPAR/ FIXHEI,THICK0,HILOECM,HILOELB,
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60 | * STEPFC,NRRUN,NSHOW,PATAPE,MONIIN,
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61 | * MONIOU,MDEBUG,NUCNUC,
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62 | * CETAPE,
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63 | * SHOWNO,ISHW,NOPART,NRECS,NBLKS,MAXPRT,NDEBDL,
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64 | * N1STTR,MDBASE,
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65 | * DEBDEL,DEBUG,FDECAY,FEGS,FIRSTI,FIXINC,FIXTAR,
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66 | * FIX1I,FMUADD,FNKG,FPRINT,FDBASE
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67 | * ,GHEISH,GHESIG
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68 | COMMON /RUNPAC/ DSN,HOST,USER
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69 | DOUBLE PRECISION FIXHEI,THICK0,HILOECM,HILOELB
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70 | REAL STEPFC
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71 | INTEGER NRRUN,NSHOW,PATAPE,MONIIN,MONIOU,MDEBUG,NUCNUC,
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72 | * SHOWNO,ISHW,NOPART,NRECS,NBLKS,MAXPRT,NDEBDL,
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73 | * N1STTR,MDBASE
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74 | INTEGER CETAPE
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75 | CHARACTER*79 DSN
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76 | CHARACTER*20 HOST,USER
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77 |
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78 | LOGICAL DEBDEL,DEBUG,FDECAY,FEGS,FIRSTI,FIXINC,FIXTAR,
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79 | * FIX1I,FMUADD,FNKG,FPRINT,FDBASE
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80 | * ,GHEISH,GHESIG
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81 | *KEND.
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82 |
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83 | DOUBLE PRECISION ALFA1,AUXIL,BETA1,COSTH3,COSTH4,CREJ,D,F1,
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84 | * EKIN,EMUON,PHI3,SCREJ,SINTH3,THETA3,U,UMAX,
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85 | * V,VC,VM,V1,W1,Z
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86 | INTEGER I
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87 | DATA ALFA1/0.625D0/
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88 | C-----------------------------------------------------------------------
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89 |
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90 | IF ( DEBUG ) WRITE(MDEBUG,444) (CURPAR(I),I=1,9)
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91 | 444 FORMAT(' MUBREM: CURPAR=',1P,9E10.3)
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92 |
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93 | C COPY COORDINATES TO SECPAR
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94 | DO 11 I = 5,8
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95 | SECPAR(I) = CURPAR(I)
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96 | 11 CONTINUE
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97 | SECPAR( 9) = GEN
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98 | C TOTAL AND KINETIC ENERGY OF MUON
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99 | EMUON = PAMA(5) * GAMMA
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100 | EKIN = EMUON - PAMA(5)
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101 | IF ( EKIN .LE. BCUT ) THEN
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102 | C MUON ENERGY IS TOO LOW TO PRODUCE BREMSSTRAHLUNG
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103 | SECPAR(2) = CURPAR(2)
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104 | GOTO 900
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105 | ENDIF
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106 | VC = BCUT/EMUON
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107 | VM = 1.D0 - CMUON(6+LT)/EMUON
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108 | IF ( VM .LE. 0.D0 ) THEN
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109 | C MAXIMUM OF BREMSSTRAHLUNG SPECTRUM IS NEGATIVE, NO BREMSSTRAHLUNG
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110 | SECPAR(2) = CURPAR(2)
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111 | GOTO 900
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112 | ENDIF
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113 | CREJ = CMUON(3+LT)/EMUON
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114 |
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115 | 50 CALL RMMAR(RD,2,1)
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116 | V = VC*(VM/VC)**RD(1)
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117 | V1 = 1.D0 - V
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118 | C COMPUTE REJECTION FUNCTION
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119 | F1 = CMUON(LT) - LOG(1.D0 + CREJ*V/V1)
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120 | SCREJ = (V1 + 0.75D0*V*V)*F1/CMUON(LT)
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121 | IF ( RD(2) .GT. SCREJ ) GOTO 50
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122 |
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123 | C PHOTON ENERGY
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124 | SECPAR(2) = EMUON * V
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125 |
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126 | C RADIATED GAMMA BELOW CUT? THEN REDUCE ENERGY OF MUON
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127 | IF ( SECPAR(2) .LE. ELCUT(4) ) THEN
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128 | GO TO 800
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129 | ENDIF
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130 |
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131 | C SET MATERIAL CONSTANTS CMUON(.) ACCORDING TO
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132 | C TARGET INDEX LT (1=N, 2=O, 3=AR) WHICH HAS BEEN SET IN BOX2
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133 | IF ( LT .EQ. 1 ) THEN
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134 | Z = 7.D0
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135 | ELSEIF ( LT .EQ. 2 ) THEN
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136 | Z = 8.D0
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137 | ELSE
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138 | Z = 18.D0
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139 | ENDIF
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140 |
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141 | C GENERATE EMITTED PHOTON ANGLES WITH RESPECT TO MUON DIRECTION
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142 | C PHI IS GENERATED ISOTROPICALLY AND THETA IS ASSIGNED A UNIVERSAL
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143 | C ANGULAR DISTRIBUTION WITH D=D(Z,E,V)
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144 | C THIS FUNCTION APPROXIMATES THE REAL DISTRIBUTION FUNCTION WHICH CAN
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145 | C BE FOUND IN: YUNG-SU TSAI, REV. MOD. PHYS. 46(1974)815
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146 | C +ERRATUM: REV. MOD. PHYS. 49(1977)421
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147 | D = 0.13D0 *(0.8D0 + 1.3D0/Z) * (100.D0 + 1.D0/EMUON) * (1.D0 + V)
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148 | W1 = 9.D0 / (9.D0 + D)
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149 | UMAX = EMUON * PI / PAMA(5)
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150 | 10 CALL RMMAR(RD,3,1)
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151 | IF ( RD(1) .LE. W1 ) THEN
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152 | BETA1 = ALFA1
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153 | ELSE
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154 | BETA1 = 3.D0 * ALFA1
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155 | ENDIF
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156 | U = -( LOG(RD(2) * RD(3)) ) / BETA1
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157 | C CUT: THETA SHOULD BE .LE. PI !
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158 | C THIS CONDITION DEPENDS ON E IN THE CASE OF D=CONST TOO!
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159 | IF ( U .GE. UMAX ) GOTO 10
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160 |
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161 | THETA3 = U * PAMA(ITYPE) / EMUON
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162 | COSTH3 = COS( THETA3 )
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163 | SINTH3 = SIN( THETA3 )
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164 | CALL RMMAR(RD,1,1)
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165 |
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166 | PHI3 = PI2 * RD(1)
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167 | CALL ADDANG( COSTHE,PHI, COSTH3,PHI3, SECPAR(3),SECPAR(4))
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168 | IF ( SECPAR(3) .GT. C(29) ) THEN
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169 | C WRITE BREMSSTRAHLUNG PHOTON TO STACK
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170 | SECPAR( 1) = 1.D0
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171 | SECPAR(10) = H
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172 | CALL TSTACK
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173 | ENDIF
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174 |
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175 | C REDUCE ENERGY OF MUON
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176 | 800 CONTINUE
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177 | EMUON = EMUON * V1
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178 | SECPAR(2) = EMUON/PAMA(5)
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179 |
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180 | 900 CONTINUE
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181 | C WRITE MUON TO STACK
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182 | SECPAR( 1) = CURPAR(1)
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183 | SECPAR( 3) = CURPAR(3)
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184 | SECPAR( 4) = CURPAR(4)
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185 | SECPAR(10) = ALEVEL
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186 | CALL TSTACK
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187 |
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188 | RETURN
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189 | END
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