1 jones 1.1 subroutine gukine
2 c
|
3 brash 1.2 c
4 c This is a subroutine to generate (x,y,theta,phi,delta-p) at
5 c the focal plane for proton from the H(e,e'p) reaction.
6 c It makes use of a simple kinematics routine, some knowledge
7 c of the extended target acceptances, and polynomials for the
8 c transport through the spectrometer from John Lerose.
|
9 jones 1.1 c
10 implicit none
11 integer ikine,itra,istak,ivert,ipart,itrtyp,napart,ipaold
12 real pkine,amass,charge,tlife,vert,pvert
13 common/gckine/ikine,pkine(10),itra,istak,ivert,ipart,itrtyp
14 + ,napart(5),amass,charge,tlife,vert(3),pvert(4),ipaold
15 integer nubuf
16 parameter (nubuf=10)
17 real ubuf(nubuf),rndm(3)
18 integer ntbeam,nttarg,nvtx
19 save nvtx
20 real plab(3),ptot,etot
21 real*8 ang,angr,phi,phir,psir
|
22 brash 1.2 real mp,ea,pa,remain
|
23 brash 1.4 real r2,r3
|
24 jones 1.1 integer nt,ierri,i0,i1,i2,i3
|
25 brash 1.2 integer i,j,k,ichoice,ichoice2,iremain
|
26 jones 1.1 real*8 rotmat,xyz(3),xyznew(3),termang
27 integer ic,ii,jj
|
28 brash 1.2 integer*4 junk1,ikinsetting
|
29 jones 1.1 real*8 xfp,yfp,tthfp,tphfp,pfp,junk2,junk3,thfp,phfp
30 real*8 e0(10),eang(10),hang(10),targ_thick(10)
|
31 brash 1.2 real*8 xtgt,ytgt,thtgt,phtgt,ptgt,dptgt
|
32 brash 1.10 real yf,ff,thetaf,dptgt2
|
33 jones 1.1 character*80 junkline
34 c
|
35 brash 1.4 c The following variables are the SIMC variables
36 c
37 real*8 x,y,z !(cm)
38 real*8 dpp !delta p/p (%)
39 real*8 dxdz,dydz !X,Y slope in spectrometer
40 real*8 x_fp,y_fp,dx_fp,dy_fp !Focal plane values to return
41 real*8 p_spec,th_spec !spectrometer setting
42 real*8 fry !vertical position@tgt (+y=down)
43 real*8 pathlen
44 logical ms_flag !mult. scattering flag
45 logical wcs_flag !wire chamber smearing flag
46 logical decay_flag !check for particle decay
47 logical ok_spec !true if particle makes it
48 real*8 resmult,m2
49 c
|
50 jones 1.1 include 'fpp_local.h'
51 include 'geant_local.h'
52 c
53 c include 'parameter.h'
54 c include 'espace_type.h'
55 c include 'detector.h'
56 c include 'transport.h'
57 c include 'option.h'
58 c
|
59 brash 1.2 common/kincom/rotmat(3,3)
60 call grndm ( rndm , 3 )
|
61 jones 1.1 c
|
62 brash 1.2 111 format(a80)
63 iremain=nevent/1000
64 remain=nevent/1000.0
65 c if(iremain.eq.remain) write(*,*)'nevent =',nevent
|
66 jones 1.1 write(*,*)'nevent =',nevent
67
68 if(nevent.eq.0) then
|
69 brash 1.2 c write(*,*)'Getting kinematics setting ...'
|
70 jones 1.1 open(unit=1,file='geant_kinematics.dat',type='UNKNOWN')
71 read(1,*)ikinsetting
72 close(unit=1)
73 open(unit=1,file='hdr_gep.dat',status='old')
74 do i=1,10
75 read(1,*)e0(i),eang(i),hang(i),targ_thick(i)
76 enddo
77 einc=e0(ikinsetting)
78 hrse_ang=eang(ikinsetting)
79 hrsh_ang=-1.0*hang(ikinsetting)
|
80 brash 1.2 trg_thk=targ_thick(ikinsetting)
|
81 jones 1.1 close(unit=1)
82 endif
83
|
84 brash 1.2 c
85 c Now we have the incident electron energy and the angles of
86 c the two spectrometers, as well as the target thickness.
87 c We need to use a) kinematics routines and b) some knowledge
88 c of the extended target acceptances to choose the x,y,theta,phi,
89 c and dpmom at the target.
90 c
91 call kincalc(einc,hrse_ang,hrsh_ang,trg_thk,xtgt,ytgt,
92 $ thtgt,phtgt,ptgt,dptgt)
93
94 c
|
95 brash 1.10 p_spec=ptgt
|
96 brash 1.2 c
|
97 brash 1.9 if(nevent.le.2)write(*,*)'******** mom = ',p_spec,' ******'
|
98 brash 1.4 c
|
99 brash 1.10 call grndm(rndm,3)
100 dptgt2=rndm(1)*0.200-0.100
101 xfp=rndm(2)*80.00-40.00
102 phfp=rndm(3)*5.0-2.5
103 c
104 call grndm(rndm,3)
105 yfp=rndm(1)*60.00-30.00
106 thfp=rndm(2)*5.0-2.5
|
107 brash 1.4 c
|
108 brash 1.8 c write(6,*)'x,phi,y,theta,ok_spec ='
109 c write(6,*)xfp,phfp,yfp,thfp,ok_spec
|
110 brash 1.4 c
111 do ii=1,20
112 ntuple_array(ii)=0.0
113 enddo
114 ntuple_array(11)=real(xfp)
115 ntuple_array(12)=real(yfp)
116 ntuple_array(13)=real(thfp)
117 ntuple_array(14)=real(phfp)
118 c
|
119 brash 1.3 pcentral=ptgt
|
120 brash 1.10 pfp=dptgt2
|
121 brash 1.4 c
|
122 brash 1.2 c Finally, we convert this information over to a format that GEANT likes.
123 c
|
124 jones 1.1
|
125 brash 1.2 1135 dpmom=pfp
126 pfp=pcentral*(1.0+pfp)
127 pmom=pfp
128 ea=sqrt(pfp**2+938.2796**2)
129 tinit=ea-938.2796
130 vert(1)=xfp
131 vert(2)=yfp
132 vert(3)=0.0
133 ntbeam = 0.0
134 nttarg = 0.0
135 ubuf(1) = 0.0
136
137 1000 continue
138 c
139 ipart = 14 ! geant pid (8=pi+,9,pi-, 14 =p)
140 ptot=pfp/1000.
|
141 jones 1.1 call grndm ( rndm , 3 )
|
142 brash 1.2 angr=thfp*3.14159265/180.0
143 phir=phfp*3.14159265/180.0
144 psir=datan(dtan(phir)*dcos(angr))
145
146 ang=thfp
147 phi=phfp
|
148 jones 1.1 c
|
149 brash 1.2 c these are the actual parameters for the track.
|
150 jones 1.1 c
|
151 brash 1.2 xinit=vert(1)
152 yinit=vert(2)
153 thinit=angr
154 phiinit=phir
155
156 c sptransport.l.particle.fp_h.ph=dtan(angr)
157 c sptransport.l.particle.fp_h.th=dtan(phir)
158 c
159 c sptransport.l.particle.fp_h.x=vert(1)/100.0
160 c
161 c sptransport.l.particle.fp_h.y=vert(2)/100.0
|
162 jones 1.1 c
163 c
|
164 brash 1.2 c next we misalign the track to simulate misalignment of the
165 c entire space frame with respect to the vdc's
|
166 jones 1.1 c
|
167 brash 1.2 c just include the translational offsets to start
|
168 jones 1.1 c
|
169 brash 1.2 c write(*,*)vert(1),vert(2),angr,phir,psir
170
171 xofff=0.0
172 yofff=0.0
173 thofff=0.0
174 phofff=0.0
175 psofff=0.0
176 c
177 c Define the inverse Euler rotation for (thofff,phiofff,psiofff)
178 c
179 c
180 rotmat(1,1)=dcos(psofff)*dcos(thofff)+dsin(psofff)*dsin(thofff)
181 $ *dsin(phofff)
182 rotmat(1,2)=-dcos(phofff)*dsin(thofff)
183 rotmat(1,3)=-dsin(psofff)*dcos(thofff)+dcos(psofff)*dsin(thofff)
184 $ *dcos(phofff)
185 rotmat(2,1)=dcos(psofff)*dsin(thofff)-dsin(psofff)*dcos(thofff)
186 $ *dsin(phofff)
187 rotmat(2,2)=dcos(phofff)*dcos(thofff)
188 rotmat(2,3)=-dsin(psofff)*dsin(thofff)-dcos(psofff)*dcos(thofff)
189 $ *dsin(phofff)
190 brash 1.2 rotmat(3,1)=dsin(psofff)*dcos(phofff)
191 rotmat(3,2)=dsin(phofff)
192 rotmat(3,3)=dcos(psofff)*dcos(phofff)
193 c
194 c
195 vert(1)=vert(1)-xofff
196 vert(2)=vert(2)-yofff
197 c
198 xyz(1)=dsin(psir)
199 xyz(2)=dcos(psir)*dsin(angr)
200 xyz(3)=dcos(psir)*dcos(angr)
201 c
202 do ic=1,3
203 xyznew(ic)=xyz(1)*rotmat(ic,1)+
204 & xyz(2)*rotmat(ic,2)+xyz(3)*rotmat(ic,3)
205 enddo
206
207 angr=datan(xyznew(2)/xyznew(3))
208 termang=xyznew(3)/dcos(angr)
209 if(termang.gt.1.0) termang=1.0
210 if(termang.lt.-1.0) termang=-1.0
211 brash 1.2 psir=dacos(termang)*abs(xyznew(1))/xyznew(1)
212 phir=datan(dtan(psir)/dcos(angr))
213
214 c write(*,*)vert(1),vert(2),angr,phir,psir
|
215 jones 1.1
216 call gsvert ( vert,ntbeam,nttarg,ubuf,0,nvtx )
|
217 brash 1.2 etot = ea - 938.2796
|
218 jones 1.1 plab(1) = ptot*dsin(psir)
219 plab(2) = ptot*dsin(angr)*dcos(psir)
220 plab(3) = ptot*dcos(angr)*dcos(psir)
|
221 brash 1.2
|
222 jones 1.1 call hfill ( 100, etot, 0., 1. )
|
223 brash 1.2
|
224 jones 1.1 call gskine ( plab,ipart,nvtx,ubuf,0,nt )
|
225 brash 1.2
|
226 jones 1.1 if ( nt.le.0 ) then
227 write ( 6,* ) ' gukine: error defining track'
228 write ( 6,* ) ' i=',i,' nt=',nt
229 stop
230 end if
|
231 brash 1.2
232 nevent=nevent+1
233
|
234 jones 1.1 return
|
235 brash 1.2
236 end
237
238 subroutine kincalc(e0,eang,hang,trg,xtgt,ytgt,
239 $ thtgt,phtgt,ptgt,dptgt)
240
241 implicit none
242
243 real*8 e0,eang,hang,trg,xtgt,ytgt,thtgt,phtgt,ptgt,dptgt
244 real*8 fg,gf
245 integer i,j,k
246 real*8 mt,mtg,mr,mpi,mn,mp,me,pi,mhe,alpha
247 real*8 escat,pscat,pcentral,thetae,phie,thetap,phip
248 real rndm(3)
249
250 fg=3.14159265/180.0
251 gf=1.0/fg
252
253 me = 0.511
254 mpi = 139.57
255 mp = 938.2796
256 brash 1.2 mn = 939.5731
257 mhe = 2808.41
258 mt = mp
259 mtg = mt/1.e3
260
261 alpha=1./137.
262
263
264 1432 call grndm ( rndm , 3 )
265 escat=mp/(1.0+mp/e0-cos(fg*eang))
266 pscat=sqrt(e0**2+escat**2-
267 $ 2.0*e0*escat*cos(fg*eang))
268 pcentral=pscat
269
270 c First, we assume that whichever are is the more backward will
271 c determine the acceptance. We then randomly choose the theta
272 c and phi for the arm that determines the acceptance within the
273 c usual full HRS acceptance and then determine from kinematics
274 c what the corresponding theta and phi are for the other arm.
275
276 if (abs(eang).gt.abs(hang)) then
|
277 brash 1.7 c phie=-.025+rndm(1)*.050
278 c thetae=-.009+rndm(2)*.018
279 if(pcentral.ge.5000) then
|
280 brash 1.9 c phie=-.00+rndm(1)*.00
281 c thetae=-.00+rndm(2)*.00
|
282 brash 1.7 phie=-.130+rndm(1)*.260
283 thetae=-.065+rndm(2)*.130
284 else if(pcentral.ge.3000.and.pcentral.lt.5000) then
285 phie=-.067+rndm(1)*.135
286 thetae=-.034+rndm(2)*.067
287 else
288 phie=-.087+rndm(1)*.174
289 thetae=-.044+rndm(2)*.087
290 endif
291 c phie=-.00+rndm(1)*.00
292 c thetae=-.00+rndm(2)*.00
|
293 brash 1.2 escat=mp/(1.0+mp/e0-cos(fg*eang+thetae)*cos(phie))
294 pscat=sqrt(e0**2+escat**2-
295 $ 2.0*e0*escat*cos(fg*eang+thetae)*cos(phie))
296 phip=dasin(escat*dsin(phie)/pscat)
297 thetap=dasin((escat*sin(fg*eang+thetae)*cos(phie))/
298 $ (pscat*cos(phip)))-fg*hang
299 else
300 c Hadron arm defining acceptance
301 1221 call grndm ( rndm, 3)
|
302 brash 1.7 phie=-.080+rndm(1)*.160
303 thetae=-.030+rndm(2)*.060
304 c phie=-.00+rndm(1)*.00
305 c thetae=-.00+rndm(2)*.00
|
306 brash 1.2 escat=mp/(1.0+mp/e0-cos(fg*eang+thetae)*cos(phie))
307 pscat=sqrt(e0**2+escat**2-
308 $ 2.0*e0*escat*cos(fg*eang+thetae)*cos(phie))
309 phip=-1.0*dasin(escat*sin(phie)/pscat)
310 thetap=dasin((escat*sin(fg*eang+thetae)*cos(phie))/
311 $ (pscat*cos(phip)))-fg*hang
312 if(abs(thetap).gt.0.030.or.abs(phip).gt.0.065) goto 1221
313 endif
314
315 ptgt=pscat
|
316 brash 1.5 c write(*,*)escat,eang,pscat,hang
|
317 brash 1.2 dptgt=(pcentral-pscat)/pcentral
|
318 jones 1.1 c
|
319 brash 1.2 c Following statement to fill just the high and low dp bins
320 c which have very low statistics. This is normally commented
321 c out.
322 c
323 c if(abs(dptgt).le.0.030) goto 1432
324 c
325 thtgt=thetap
326 phtgt=phip
327 xtgt=0.0
328 ytgt=0.0
329
330 return
|
331 jones 1.1 end
|