1 |
cafagna |
1.1 |
* |
2 |
pamela |
1.2 |
* $Id: gpgig.F,v 1.1 2005/12/20 12:21:05 cafagna Exp $ |
3 |
|
|
* |
4 |
|
|
* $Log: gpgig.F,v $ |
5 |
|
|
* Revision 1.1 2005/12/20 12:21:05 cafagna |
6 |
|
|
* gpnd directory added along with ND files |
7 |
cafagna |
1.1 |
* |
8 |
|
|
* Revision 3.1.1.1 2002/07/11 16:02:00 cafagna |
9 |
|
|
* First GPAMELA release on CVS |
10 |
|
|
* |
11 |
|
|
* |
12 |
|
|
*CMZ : 3.00/00 11/05/2001 13.44.09 by Marialuigia Ambriola |
13 |
|
|
*CMZ : 2.01/00 05/04/2000 14.35.18 by Marialuigia Ambriola |
14 |
|
|
*CMZ : 2.00/00 03/03/2000 15.39.05 by Francesco Cafagna |
15 |
|
|
*CMZ : 1.01/00 30/04/96 18.28.33 by Francesco Cafagna |
16 |
|
|
*CMZ : 1.00/03 29/04/96 16.56.08 by Francesco Cafagna |
17 |
|
|
*-- Author : Francesco Cafagna 29/04/96 |
18 |
|
|
SUBROUTINE GPGIG |
19 |
|
|
************************************************************************ |
20 |
|
|
* * |
21 |
|
|
* User action in GUSTEP * |
22 |
|
|
* * |
23 |
|
|
* Variables definition: * |
24 |
|
|
* IN: * |
25 |
|
|
* IFLAG = 1, just entered GUSTEP * |
26 |
|
|
* IFLAG = 2, leaving GUSTEP * |
27 |
|
|
* * |
28 |
|
|
* Called by: GUSTEP * |
29 |
|
|
* Author: Francesco Cafagna, 29/04/96 16.56.08 * |
30 |
|
|
* * |
31 |
|
|
************************************************************************ |
32 |
|
|
#include "gctmed.inc" |
33 |
|
|
#include "gcking.inc" |
34 |
|
|
#include "gctrak.inc" |
35 |
pamela |
1.2 |
#include "gckine.inc" |
36 |
|
|
#include "gpgig.inc" |
37 |
|
|
#include "gpgneut.inc" |
38 |
cafagna |
1.1 |
* |
39 |
|
|
LOGICAL W,GPLOOK |
40 |
|
|
INTEGER IFLAG |
41 |
|
|
INTEGER IFL,IN,MECNAM(MAXMEC) |
42 |
pamela |
1.2 |
c$$$ IN = INWVOL |
43 |
|
|
c$$$ IF(IN.NE.0) RETURN |
44 |
|
|
|
45 |
|
|
IF ((GETOT.GT.0.009097).AND.(GETOT.LT.0.028608) |
46 |
|
|
+ .AND.IPART.EQ.1) THEN |
47 |
cafagna |
1.1 |
* |
48 |
pamela |
1.2 |
* Call the Gigantic resonance routine. |
49 |
|
|
* |
50 |
|
|
CALL GPGRES(STEP,GETOT,VECT(4)*VECT(7), |
51 |
|
|
+ VECT(5)*VECT(7),VECT(6)*VECT(7)) |
52 |
|
|
* |
53 |
|
|
* First of all let's stop the gamma tracking if neutron(s) is(are) generated |
54 |
|
|
* |
55 |
|
|
IF(Number_N.gt.0) THEN |
56 |
|
|
ISTOP = 1 |
57 |
|
|
DO I=1,Number_n |
58 |
|
|
* |
59 |
|
|
* Increment the produced secondaries number |
60 |
|
|
* |
61 |
|
|
NGKINE = NGKINE + 1 |
62 |
|
|
* |
63 |
|
|
* Store the mechnism number |
64 |
|
|
* |
65 |
|
|
KASE = IGMEC |
66 |
|
|
* |
67 |
|
|
* Store the secondaries position in the GCKING common |
68 |
|
|
* |
69 |
|
|
GPOS(1,NGKINE) = VECT(1) |
70 |
|
|
GPOS(2,NGKINE) = VECT(2) |
71 |
|
|
GPOS(2,NGKINE) = VECT(3) |
72 |
|
|
* |
73 |
|
|
* Now the other parameters: px, py, pz, E, Particle ID, TOF |
74 |
|
|
* |
75 |
|
|
GKIN(1,NGKINE) = SQRT(NEUT_EN(I)**2-AMGIG**2)* |
76 |
|
|
+ SIN(TETA_N(I))*COS(FI_N(I)) |
77 |
|
|
GKIN(2,NGKINE) = SQRT(NEUT_EN(I)**2-AMGIG**2)* |
78 |
|
|
+ SIN(TETA_N(I))*SIN(FI_N(I)) |
79 |
|
|
GKIN(3,NGKINE) = SQRT(NEUT_EN(I)**2-AMGIG**2)* |
80 |
|
|
+ COS(TETA_N(I)) |
81 |
|
|
GKIN(4,NGKINE) = NEUT_EN(I) |
82 |
|
|
GKIN(5,NGKINE) = IPGIG |
83 |
|
|
TOFD(NGKINE) = TOFG |
84 |
|
|
ENDDO |
85 |
|
|
ENDIF |
86 |
cafagna |
1.1 |
ENDIF |
87 |
pamela |
1.2 |
999 CONTINUE |
88 |
|
|
|
89 |
cafagna |
1.1 |
RETURN |
90 |
|
|
END |
91 |
pamela |
1.2 |
|