13 if(emu .le. mubremin)
then 15 elseif(emu .le. mubremax1)
then 17 call kintp3(mubrtx, 1, mubrtxt, mubrlemin,
18 * mubrdetx, ale, prob)
21 prob = mubrtx(mubrtxt)
42 real*8 vc, vmx, cmuvmax2, term1, term2, u1, u2, x
43 real*8 delta, logf, func, u, v
47 term1 =4.
d0/3.
d0 * (log(vmx/vc) - (vmx-vc))
48 term2 = (vmx-vc)*(vmx+vc)/2.
d0 52 if(u .le. term1/(term1+term2))
then 59 if( u .lt. (1.0-x))
then 60 if(x .lt. vmx)
goto 10
70 if(x .gt. vc .and. x .lt. vmx)
goto 20
79 delta = (
masmu/emu) * v /(1.
d0-v)/2
80 logf = muakm / (1.
d0 + muakm2*delta)
81 if(zeff .gt. 10.)
then 82 logf = logf * 2./3.
d0 /zeff3
86 if(u .gt. func/
mulogf0)
goto 100
block data cblkElemag data *AnihiE ! Eposi< 1 TeV, anihilation considered *X0/365.667/, ! radiation length of air in kg/m2 *Ecrit/81.e-3/, ! critical energy of air in GeV *MaxComptonE/1./, ! compton is considered below 1 GeV *MaxPhotoE/1.e-3/, ! above this, PhotoElectric effect neg. *MinPhotoProdE/153.e-3/, ! below 153 MeV, no gp --> hadrons ! scattering const not MeV *Knockon true
subroutine cmubrsmpp(Emu, prob, path)
subroutine cmubrsmpe(Emu, Eg)
block data cblkEvhnp ! currently usable models data RegMdls ad *special data *Cekaon d0
subroutine kintp3(f, intv, n, x1, h, x, ans)
! muon interaction related variables ! real Zeff3 ! Zeff **real muPrEmax1 integer muPrTXT ! real muBrEmax1 integer muBrTXT ! real muNEmax1 integer muNTXT ! real muNpwdEdxt real real mulogf0 real muBrLEmin common muintc mulogf0