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brem.f
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! BREM.FOR
! Exact soft photon bremstrahlung calculation of
! delta, delta^\prime, and exponentiations thereof
real*8 function brem(ein,eout,egamma,radiate_proton,bsoft,bhard,dbsoft)
implicit none
include 'brem.inc'
real*8 pi, am, ame, e2
parameter (pi=3.141592653589793)
parameter (am= .93827231)
parameter (ame= .00051099906)
parameter (e2= 1./137.0359895)
real*8 ein ! electron energy
real*8 eout ! final electron energy
real*8 egamma ! energy of bremsstrahling photon
real*8 eang,ak,akp,ap,pang,eta,ape
real*8 q2,de
real*8 aprod,adot,ar1,ar2,alpha
real*8 bpi,bpf,bpp,bei,bef,bee,bepii,bepif,bepfi,bepff
real*8 dbpi,dbpf,dbpp,dbei,dbef,dbee,dbepii,dbepif,dbepfi,
> dbepff !derivatives of b's
real*8 b,bz,bzz,db,dbz,dbzz,bhard,bsch,spence,bsoft,dbsoft
real*8 inter
logical radiate_proton
! Convert to GeV
ak=ein/1000.
akp=eout/1000.
de=egamma/1000.
! electron scattering angle
eang= 2.*asin((am/(2.*ak)*(ak/akp-1.))**0.5)
eta= 1.+2.*ak*sin(eang/2.)**2/am
q2= 4.*ak*akp*sin(eang/2.)**2
! final proton energy/momentum/scattering angle.
ape= am+ak-akp
ap= sqrt(ape**2-am**2)
pang= acos((ak-akp*cos(eang))/ap)
if(produce_output) then
write(6,*)' q2 ',q2
write(6,*)' k ',ak
write(6,*)' kp ',akp
write(6,*)' eang ',eang*180./pi
write(6,*)' ap ',ap
write(6,*)' pang ',pang*180./pi
write(6,*)' eta ',eta
endif
! Calculate components of delta soft
! ... electron terms
! direct initial electron
aprod= 1.e0
bei= aprod*(-1./(2.*pi))*log(ak/de)
dbei= aprod*(1./(2.*pi*de))
! direct final electron
aprod= 1.e0
bef= aprod*(-1./(2.*pi))*log(akp/de)
dbef= aprod*(1./(2.*pi*de))
! e-e interference
aprod= -1.e0
adot= ak*akp*(1.-cos(eang))
alpha= 2.*ame**2-2.*adot
ar1= 0.5+sqrt(adot**2-ame**4)/alpha
ar2= 0.5-sqrt(adot**2-ame**4)/alpha
bee= aprod*adot*inter(calculate_spence,alpha,ar1,ar2,ak,akp,de)
dbee= aprod*adot/(pi*alpha*(ar1-ar2)*de)*
> (log((ar1-1)/ar1)-log((ar2-1)/ar2))
if(produce_output) write(6,*) ar1,ar2
! ... proton terms
if (radiate_proton) then
! initial p direct
aprod= 1.e0
bpi= aprod*(-1./(2.*pi))*log(am/de)
dbpi= aprod*(1./(2.*pi*de))
! final p direct
aprod= 1.e0
bpf= aprod*(-1./(2.*pi))*log(ape/de)
dbpf= aprod*(1/(2.*pi*de))
! p-p interference
aprod= -1.e0
adot= am*ape
alpha= 2.*am**2-2.*adot
ar1= 0.5+sqrt(adot**2-am**4)/alpha
ar2= 0.5-sqrt(adot**2-am**4)/alpha
bpp= aprod*adot*inter(calculate_spence,alpha,ar1,ar2,am,ape,de)
dbpp= aprod*adot/(pi*alpha*(ar1-ar2)*de)*
> (log((ar1-1)/ar1)-log((ar2-1)/ar2))
if(produce_output) write(6,*) ar1,ar2
! ei-pi interference
aprod= -1.e0
adot= ak*am
alpha= am**2+ame**2-2.*adot
ar1= (am**2-adot+sqrt(adot**2-(ame*am)**2))/alpha
ar2= (am**2-adot-sqrt(adot**2-(ame*am)**2))/alpha
bepii= aprod*adot*inter(calculate_spence,alpha,ar1,ar2,ak,am,de)
dbepii= aprod*adot/(pi*alpha*(ar1-ar2)*de)*
> (log((ar1-1)/ar1)-log((ar2-1)/ar2))
if(produce_output) write(6,*) ar1,ar2
! ef-pf interference
aprod= -1.e0
adot= akp*ape-akp*ap*cos(eang+pang)
alpha= am**2+ame**2-2.*adot
ar1= (am**2-adot+sqrt(adot**2-(ame*am)**2))/alpha
ar2= (am**2-adot-sqrt(adot**2-(ame*am)**2))/alpha
bepff= aprod*adot*inter(calculate_spence,alpha,ar1,ar2,akp,ape,de)
dbepff= aprod*adot/(pi*alpha*(ar1-ar2)*de)*
> (log((ar1-1)/ar1)-log((ar2-1)/ar2))
if(produce_output) write(6,*) ar1,ar2
! ei-pf interference
aprod= 1.e0
adot= ak*ape-ak*ap*cos(pang)
alpha= am**2+ame**2-2.*adot
ar1= (am**2-adot+sqrt(adot**2-(ame*am)**2))/alpha
ar2= (am**2-adot-sqrt(adot**2-(ame*am)**2))/alpha
bepif= aprod*adot*inter(calculate_spence,alpha,ar1,ar2,ak,ape,de)
dbepif= aprod*adot/(pi*alpha*(ar1-ar2)*de)*
> (log((ar1-1)/ar1)-log((ar2-1)/ar2))
if(produce_output) write(6,*) ar1,ar2
! ef-pi interference
aprod= 1.e0
adot= akp*am
alpha= am**2+ame**2-2.*adot
ar1= (am**2-adot+sqrt(adot**2-(ame*am)**2))/alpha
ar2= (am**2-adot-sqrt(adot**2-(ame*am)**2))/alpha
bepfi= aprod*adot*inter(calculate_spence,alpha,ar1,ar2,akp,am,de)
dbepfi= aprod*adot/(pi*alpha*(ar1-ar2)*de)*
> (log((ar1-1)/ar1)-log((ar2-1)/ar2))
if(produce_output) write(6,*) ar1,ar2
endif ! <radiate_proton>
! All together now!
b= 2.*e2*(bei+bef+bee)
if (radiate_proton) then
bzz= 2.*e2*(bpi+bpf+bpp)
bz= 2.*e2*(bepii+bepff+bepif+bepfi)
else
bzz = 0.0
bz = 0.0
endif
bsoft=b+bz+bzz
bhard= -1.*(e2/pi)*(-28/9.+13./6.*log(q2/ame**2))
db= 2.*e2*(dbei+dbef+dbee)
if (radiate_proton) then
dbzz= 2.*e2*(dbpi+dbpf+dbpp)
dbz= 2.*e2*(dbepii+dbepff+dbepif+dbepfi)
else
dbzz = 0.0
dbz = 0.0
endif
dbsoft= db+dbz+dbzz
if(produce_output) then
write(6,*)' ----- results ----- '
write(6,*)' b= ',b
write(6,*)' bz= ',bz
write(6,*)' bzz= ',bzz
write(6,*)' bhard= ',bhard
write(6,*)' total= ',bsoft+bhard
write(6,*)' exp= ',1.-exp(-1.*(bsoft))*(1.-bhard)
write(6,*)' '
write(6,*)' ultra-relativistic limit'
call srad(ak,akp,eang,q2,ame,am,ap,de,produce_output)
write(6,*)' Schwinger Result'
bsch= 2.*e2/pi*((log(ak/de)-13./12.)*(log(q2/ame**2)-1.)+17./36.+
> 0.5*(pi**2/6.-spence((cos(eang/2.))**2)))
write(6,*)' b= ',bsch
endif
! ... and the result --> the value of the radiative cross-section,
! dsigma/dEgamma = -dbsoft * exp(-bsoft) * (1-bhard)
! ......... the derivative has dimension 1/[energy] --> convert back to MeV
dbsoft = dbsoft/1000.
if (exponentiate) then
brem = -dbsoft/exp(bsoft)
else
brem = 1.-dbsoft
endif
if (include_hard) brem = brem*(1.-bhard)
return
end
!-----------------------------------
real*8 function inter(calculate_spence,alpha,ar1,ar2,e1,e2,de)
! explicit evaluation of integral ... may or may not ignore spence functions
implicit none
real*8 pi
parameter (pi=3.141592653589793)
real*8 alpha,ar1,ar2,e1,e2,de
real*8 de2,amult,arg1,arg2,arg3,arg4,spence
logical calculate_spence
de2 = e1-e2
amult = -1./(alpha*(ar1-ar2))
inter = log(abs((e2/de)+ar1*(de2/de)))*log(abs((ar1-1.)/ar1)) -
> log(abs((e2/de)+ar2*(de2/de)))*log(abs((ar2-1.)/ar2))
if (calculate_spence) then
arg1= (de2/(e2+ar1*de2))*(ar1-1.)
arg2= (de2/(e2+ar1*de2))*(ar1)
arg3= (de2/(e2+ar2*de2))*(ar2-1.)
arg4= (de2/(e2+ar2*de2))*(ar2)
inter = inter - spence(arg1)+spence(arg2)+spence(arg3)-spence(arg4)
endif
inter= inter*amult/(pi)
return
end
!-----------------------------------
subroutine srad(ak,akp,eang,q2,ame,am,ap,de,produce_output)
! calculates ultra-relativistic limit
implicit none
real*8 pi, alpha
parameter (pi = 3.141592653589793)
parameter (alpha = 1./137.0359895)
real*8 ak,akp,eang,q2,ame,am,ap
real*8 eta,dsoft,dhard,de
real*8 dsoftz,dsoftzz,ep
logical produce_output
ep= sqrt(ap**2+am**2)
dhard= -13./12.*(log(q2/ame**2)-1.)+17./36.
eta= 1.+2.*ak*(sin(eang/2.)**2)/am
dsoft= alpha/pi*log(ak*akp/de**2)*(log(q2/ame**2)-1.)
dsoftz= alpha/pi*log(eta)*(log(ak*akp/de**2)+log(am*ep/de**2))
dsoftzz= alpha/pi*log(am*ep/de**2)*(log(q2/am**2)-1.)
if(dsoftzz.le.0) dsoftzz=0.0
if (produce_output) then
write(6,*)' '
write(6,*)' b= ',dsoft
write(6,*)' bz= ',dsoftz
write(6,*)' bzz= ',dsoftzz
endif
return
end
!-----------------------------------
real*8 function spence(ax)
implicit none
real*8 pi
parameter (pi=3.141592653589793)
real*8 ax,bx
bx= abs(ax)
! ... N.B. Have replaced the former calculation (commented out) with an
! ... approximate expression -- saves a WHALE of CPU!
!
! if(bx.lt.1) then
! spence= ssum(ax,100)
! else if (ax.gt.1) then
! spence= -0.5*(log(bx))**2+pi**2/3.-ssum(1./ax,100)
! else if (ax.le.-1) then
! spence= -0.5*(log(bx))**2-pi**2/6.-ssum(1./ax,100)
! else if (ax.eq.1) then
! spence= pi**2/6.
! else if (ax.eq.-1) then
! spence= -pi**2/12.
! endif
if (bx.le.1) then
spence = 0.0
else
spence = -0.5*(log(bx))**2
endif
return
end
!-----------------------------------
real*8 function ssum(as,n)
implicit none
integer n,i
real*8 as
ssum= 0.0
if(as.ne.0) then
if(n.ge.10000) write(6,*)' large n in function ssum (brem.f)'
do i= 1,n
ssum= ssum+as**i/(1.*i)**2
enddo
endif
return
end
!------------------------------------------------------------------------------
real*8 function bremos(egamma, ! photon energy
> k_ix, k_iy, k_iz, ! incoming electron 3-momentum
> k_fx, k_fy, k_fz, ! scattered electron 3-momentum
> p_ix, p_iy, p_iz, ! incoming proton 3-momentum (pm)
> p_fx, p_fy, p_fz, p_fe, ! scattered proton 4-momentum
> radiate_proton, ! proton radiation flag
> bsoft, bhard, dbsoft)
! Calculation of soft photon radiative correction factor and its derivative
! allowing for both initial and final protons to be offshell.
! conventions identical to on-shell calculation
implicit none
include 'brem.inc'
real*8 pi, twopi, ame, e2, mp
parameter (pi=3.141592653589793)
parameter (twopi=2.*pi)
parameter (ame= .00051099906)
parameter (e2= 1./137.0359895)
parameter (mp= .93827231)
type four_vector
real*8 e, x, y, z
end type
real*8 egamma, de
real*8 k_ix,k_iy,k_iz
real*8 k_fx,k_fy,k_fz
real*8 p_ix,p_iy,p_iz
real*8 p_fx,p_fy,p_fz,p_fe
real*8 ami,amf,q2
real*8 aprod,adot,ar1,ar2,alpha
real*8 bpi,bpf,bpp,bei,bef,bee,bepii,bepif,bepfi,bepff
real*8 dbpi,dbpf,dbpp,dbei,dbef,dbee,dbepii,dbepif,
> dbepfi,dbepff !derivatives of b's
real*8 b,bz,bzz,db,dbz,dbzz
real*8 bsoft,bhard,dbsoft,bsch
real*8 inter,inter_prime
logical radiate_proton
type(four_vector):: k_i, k_f, p_i, p_f
! Initialize
! ... put input into local variables, while converting energies/momenta to GeV.
de = egamma/1000.
k_i%x = k_ix/1000.
k_i%y = k_iy/1000.
k_i%z = k_iz/1000.
k_f%x = k_fx/1000.
k_f%y = k_fy/1000.
k_f%z = k_fz/1000.
p_i%x = p_ix/1000.
p_i%y = p_iy/1000.
p_i%z = p_iz/1000.
p_f%e = p_fe/1000.
p_f%x = p_fx/1000.
p_f%y = p_fy/1000.
p_f%z = p_fz/1000.
! ... compute electron energies
k_i%e= (k_i%x**2+k_i%y**2+k_i%z**2+ame**2)**0.5
k_f%e= (k_f%x**2+k_f%y**2+k_f%z**2+ame**2)**0.5
! ........ if he insists on e-m conservation like below, just compute p_i.e
c p_i%e = k_f%e+p_f%e-k_i%e
p_i%e = mp
! ... check energy-momentum conservation
! e_check= abs(k_f%e+p_f%e-k_i%e-p_i%e)
! x_check= abs(k_f%x+p_f%x-k_i%x-p_i%x)
! y_check= abs(k_f%y+p_f%y-k_i%y-p_i%y)
! z_check= abs(k_f%z+p_f%z-k_i%z-p_i%z)
!
! if((e_check.gt.0.0001).or.(x_check.gt.0.0001).or.
! + (y_check.gt.0.0001).or.(z_check.gt.0.0001)) then
! write(6,*)' bad kinematics'
! return
! endif
! ... compute Q2 and masses of initial and final protons
q2=-1.*( (k_f%e-k_i%e)**2-(k_f%x-k_i%x)**2-
> (k_f%y-k_i%y)**2-(k_f%z-k_i%z)**2)
if (produce_output) write(6,*)' q2= ',q2
c ami= ((p_i%e)**2-(p_i%x)**2-(p_i%y)**2-(p_i%z)**2)**0.5
ami= mp
amf= ((p_f%e)**2-(p_f%x)**2-(p_f%y)**2-(p_f%z)**2)**0.5
! Calculate components of delta soft
! ... electron terms
! ........ direct initial electron
aprod= 1.e0
bei= aprod*(-1./twopi)*log(k_i%e/de)
dbei= aprod*(-1./twopi)*(-1./de)
! ........ direct final electron
aprod= 1.e0
bef= aprod*(-1./twopi)*log(k_f%e/de)
dbef= aprod*(-1./twopi)*(-1./de)
! ........ e-e interference
aprod= -1.e0
adot= k_i%e*k_f%e-k_i%x*k_f%x-k_i%y*k_f%y-k_i%z*k_f%z
alpha= 2.*ame**2-2.*adot
ar1= 0.5+sqrt(4.*adot**2-4.*ame**4)/(2.*alpha)
ar2= 0.5-sqrt(4.*adot**2-4.*ame**4)/(2.*alpha)
bee= aprod*adot*inter(calculate_spence,alpha,ar1,ar2,k_i%e,k_f%e,de)
dbee= aprod*adot*inter_prime(alpha,ar1,ar2,de)
if (produce_output) write(6,*) ar1,ar2
! ... proton terms
if (radiate_proton) then
! ........ initial p direct
aprod= 1.e0
bpi= aprod*(-1./twopi)*log(p_i%e/de)
dbpi= aprod*(-1./twopi)*(-1./de)
! ........ final p direct
aprod= 1.e0
bpf= aprod*(-1./twopi)*log(p_f%e/de)
dbpf= aprod*(-1./twopi)*(-1./de)
! ........ p-p interference
aprod= -1.e0
adot= p_i%e*p_f%e-p_i%x*p_f%x-p_i%y*p_f%y-p_i%z*p_f%z
alpha= ami**2+amf**2-2.*adot
ar1= (2.*amf**2-2.*adot+sqrt(4.*adot**2-4.*(ami*amf)**2))/(2.*alpha)
ar2= (2.*amf**2-2.*adot-sqrt(4.*adot**2-4.*(ami*amf)**2))/(2.*alpha)
bpp= aprod*adot*inter(calculate_spence,alpha,ar1,ar2,p_i%e,p_f%e,de)
dbpp= aprod*adot*inter_prime(alpha,ar1,ar2,de)
if (produce_output) write(6,*) ar1,ar2
! ........ ei-pi interference
aprod= -1.e0
adot= k_i%e*p_i%e-k_i%x*p_i%x-k_i%y*p_i%y-k_i%z*p_i%z
alpha= ami**2+ame**2-2.*adot
ar1= (2.*ami**2-2.*adot+sqrt(4.*adot**2-4.*(ame*ami)**2))/(2.*alpha)
ar2= (2.*ami**2-2.*adot-sqrt(4.*adot**2-4.*(ame*ami)**2))/(2.*alpha)
bepii= aprod*adot*inter(calculate_spence,alpha,ar1,ar2,k_i%e,p_i%e,de)
dbepii= aprod*adot*inter_prime(alpha,ar1,ar2,de)
if (produce_output) write(6,*) ar1,ar2
! ........ ef-pf interference
aprod= -1.e0
adot= k_f%e*p_f%e-k_f%x*p_f%x-k_f%y*p_f%y-k_f%z*p_f%z
alpha= amf**2+ame**2-2.*adot
ar1= (2.*amf**2-2.*adot+sqrt(4.*adot**2-4.*(ame*amf)**2))/(2.*alpha)
ar2= (2.*amf**2-2.*adot-sqrt(4.*adot**2-4.*(ame*amf)**2))/(2.*alpha)
bepff= aprod*adot*inter(calculate_spence,alpha,ar1,ar2,k_f%e,p_f%e,de)
dbepff= aprod*adot*inter_prime(alpha,ar1,ar2,de)
if (produce_output) write(6,*) ar1,ar2
! ........ ei-pf interference
aprod= 1.e0
adot= k_i%e*p_f%e-k_i%x*p_f%x-k_i%y*p_f%y-k_i%z*p_f%z
alpha= amf**2+ame**2-2.*adot
ar1=(2.*amf**2-2.*adot+sqrt(4.*adot**2-4.*(ame*amf)**2))/(2.*alpha)
ar2=(2.*amf**2-2.*adot-sqrt(4.*adot**2-4.*(ame*amf)**2))/(2.*alpha)
bepif= aprod*adot*inter(calculate_spence,alpha,ar1,ar2,k_i%e,p_f%e,de)
dbepif= aprod*adot*inter_prime(alpha,ar1,ar2,de)
if (produce_output) write(6,*) ar1,ar2
! ........ ef-pi interference
aprod= 1.e0
adot= k_f%e*p_i%e-k_f%x*p_i%x-k_f%y*p_i%y-k_f%z*p_i%z
alpha= ami**2+ame**2-2.*adot
ar1=(2.*ami**2-2.*adot+sqrt(4.*adot**2-4.*(ame*ami)**2))/(2.*alpha)
ar2=(2.*ami**2-2.*adot-sqrt(4.*adot**2-4.*(ame*ami)**2))/(2.*alpha)
bepfi= aprod*adot*inter(calculate_spence,alpha,ar1,ar2,k_f%e,p_i%e,de)
dbepfi= aprod*adot*inter_prime(alpha,ar1,ar2,de)
if (produce_output) write(6,*) ar1,ar2
endif ! <radiate_proton>
! All together now!
b= 2.*e2*(bei+bef+bee)
if (radiate_proton) then
bzz= 2.*e2*(bpi+bpf+bpp)
bz= 2.*e2*(bepii+bepff+bepif+bepfi)
else
bzz = 0.0
bz = 0.0
endif
bsoft = b + bz + bzz
bhard= -1.*(e2/pi)*(-28/9.+13./6.*log(q2/ame**2))
* bhard= (e2/pi)*(2-1.5*log(q2/ame**2))
* bhard= bhard+vac(q2)
db= 2.*e2*(dbei+dbef+dbee)
if (radiate_proton) then
dbzz= 2.*e2*(dbpi+dbpf+dbpp)
dbz= 2.*e2*(dbepii+dbepff+dbepif+dbepfi)
else
dbzz = 0.0
dbz = 0.0
endif
dbsoft= db+dbz+dbzz
if (produce_output) then
write(6,*)' ----- results ----- '
write(6,*)' b+bhard= ',b+bhard
write(6,*)' bz= ',bz
write(6,*)' bzz= ',bzz
write(6,*)' bhard= ',bhard
write(6,*)' total= ',1-bsoft-bhard
write(6,*)' exp= ',exp(-1.*(bsoft))*(1.-bhard)
write(6,*)' 1-bhard= ',1-bhard
write(6,*)' exps= ',exp(-1.*(bsoft))
write(6,*)' expse= ',exp(-1.*b)
write(6,*)' expsp= ',exp(-1.*(bz+bzz))
write(6,*)' '
write(6,*)' Schwinger Result'
bsch= 2.*e2/pi*((log(k_i%e/de)-13./12.)*(log(q2/ame**2)-1.)+17./36.)
write(6,*)' b= ',bsch
endif
! ... and the result --> the value of the radiative cross-section,
! dsigma/dEgamma = -dbsoft * exp(-bsoft) * (1-bhard)
! ......... the derivative has dimension 1/[energy] --> convert back to MeV
dbsoft = dbsoft/1000. !convert back to MeV
if (exponentiate) then
bremos = -dbsoft/exp(bsoft)
else
bremos = 1.-dbsoft
endif
if (include_hard) bremos = bremos*(1.-bhard)
return
end
!-----------------------------------
c
c explicit evaluation of DERIVATIVE of integral (wrt de)
c
real*8 function inter_prime(alpha,ar1,ar2,de)
implicit none
real*8 pi
parameter (pi=3.141592653589793)
real*8 alpha,ar1,ar2,de
real*8 amult
amult = -1./(alpha*(ar1-ar2))
inter_prime = (-1./de)*amult/pi*
> (log(abs((ar1-1.)/ar1))-log(abs((ar2-1.)/ar2)))
return
end
!-----------------------------------
real*8 function vac(q2)
implicit none
real*8 q2
real*8 am(10),ae(10)
real*8 dele,dell
integer*4 j
real*8 del
am(1)= 0.00051099906
ae(1) = 1.0
am(2)= .1057
ae(2)= 1.0
am(3)= 1.782
ae(3)= 1.0
am(4)= 0.3
ae(4)= 2./3.
am(5)= .3
ae(5)= 1./3.
am(6)= .430
ae(6)= 1./3.
am(7)= 1.5
ae(7)= 2./3.
am(8)= 5.
ae(8)= 1./3.
dele= del(q2,am(1),ae(1))
dell= 0.0
do 20 j= 1,3
dell= dell+del(q2,am(j),ae(j))
20 continue
vac= dell
return
end
!-----------------------------------
real*8 function del(q2,bm,be)
implicit none
real*8 q2,bm,be
real*8 x,alpha
x= 4.*bm**2/q2
alpha= be**2/137.0359895
del= -2.*alpha/(3.*3.14159265)*(-5./3.+x+(1-x/2)*(1+x)**0.5*
> log(((1+x)**0.5+1)/((1+x)**0.5-1)))
return
end