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fe4da5cc | 1 | * |
2 | * $Id$ | |
3 | * | |
4 | * $Log$ | |
5 | * Revision 1.1.1.1 1995/10/24 10:21:46 cernlib | |
6 | * Geant | |
7 | * | |
8 | * | |
9 | #include "geant321/pilot.h" | |
10 | *CMZ : 3.21/03 07/10/94 18.41.50 by S.Giani | |
11 | *-- Author : | |
12 | SUBROUTINE GUHADR | |
13 | C. | |
14 | C. ****************************************************************** | |
15 | C. * * | |
16 | C. * User routine to generate one hadronic interaction * | |
17 | C. * * | |
18 | C. * ==>Called by : GTHADR,GTNEUT * | |
19 | C. * * | |
20 | C. ****************************************************************** | |
21 | C. | |
22 | *======================================================================* | |
23 | * * | |
24 | * An interface with a part of the FLUKA shower code is available in * | |
25 | * GEANT 3.21. The following conditions and warnings must be taken * | |
26 | * into account when using the FLUKA routines. * | |
27 | * * | |
28 | *======================================================================* | |
29 | *======================================================================* | |
30 | * * | |
31 | * FFFF L U U K K AA * | |
32 | * F L U U K K A A * | |
33 | * FFF L U U KK AAAA * | |
34 | * F L U U K K A A * | |
35 | * F LLLL UU K K A A * | |
36 | * * | |
37 | * (C) Copyright of the authors * | |
38 | * * | |
39 | * A. Fasso'*, A. Ferrari#, J. Ranft$, P.R. Sala# * | |
40 | * * | |
41 | * *: CERN, #: INFN -Milan, $: CERN/Frascati * | |
42 | * * | |
43 | * (e-mail: FERRARIA@CERNVM.CERN.CH) * | |
44 | * * | |
45 | *======================================================================* | |
46 | * * | |
47 | * - All the rights concerning FLUKA or parts of it are only of the * | |
48 | * authors and are independent from those of the GEANT code * | |
49 | * * | |
50 | * - FLUKA [1-6] is a standalone code capable of simulating the inter-* | |
51 | * action and transport of all components of EM and hadronic cas- * | |
52 | * cades up to several TeV. However, only cross sections and * | |
53 | * models for hadronic elastic and inelastic interactions (end 1992 * | |
54 | * status) are included in this GEANT version. * | |
55 | * * | |
56 | * - The most recent FLUKA model [4,6] for nucleon and pion interac- * | |
57 | * tions in the intermediate energy range is not fully implemented * | |
58 | * in GEANT. Only a simplified version, limited to p and n below * | |
59 | * 250 MeV, is available in GEANT 3.21. A coarser model is used for * | |
60 | * other projectiles in this energy range. However the implemented * | |
61 | * parts should be adequate for most detector simulations and sim- * | |
62 | * ilar applications for which GEANT is generally used. Their accu- * | |
63 | * racy could be insufficient for some nuclear physics studies or * | |
64 | * demanding simulations at low energies, where the more sophistic- * | |
65 | * ated models [4,6] could be required. * | |
66 | * * | |
67 | * - The performances of GEANT-FLUKA are therefore not representative * | |
68 | * of those of FLUKA standalone and should be referenced as such * | |
69 | * rather than simply GEANT or FLUKA. * | |
70 | * * | |
71 | * - The authors reserve the right of publishing about the physical * | |
72 | * models developed for FLUKA. Running the FLUKA routines in isol- * | |
73 | * ation for benchmarks (or equivalent use) is not permitted, * | |
74 | * except after consultations or in collaboration with the authors. * | |
75 | * * | |
76 | * - The FLUKA routines are supposed to be included and used in * | |
77 | * GEANT only. Any other use must be authorized by the authors. * | |
78 | * * | |
79 | * - References: at least reference [5] should be always quoted when * | |
80 | * reporting results obtained with GEANT-FLUKA * | |
81 | * * | |
82 | * [1] A. Fasso', A. Ferrari, J. Ranft, P. R. Sala, G. R. Stevenson and * | |
83 | * J. M. Zazula, "FLUKA92", presented at the workshop on "Simulat- * | |
84 | * ing Accelerator Radiation Environment", SARE, Santa Fe, 11-15 * | |
85 | * january (1993), Proceedings in press. * | |
86 | * * | |
87 | * [2] P.A. Aarnio, A. Fasso', A. Ferrari, J.-H. Moehring, J. Ranft, * | |
88 | * P.R. Sala, G.R. Stevenson and J.M. Zazula, Proc. MC93 Int. Conf. * | |
89 | * on Monte-Carlo Simulation in High-Energy and Nuclear Physics, * | |
90 | * Tallahassee, Florida, 22-26 february (1993), World Scientific, * | |
91 | * p. 88 (1994). * | |
92 | * * | |
93 | * [3] P.A. Aarnio, A. Fasso', A. Ferrari, J.-H. Moehring, J. Ranft, * | |
94 | * P.R. Sala, G.R. Stevenson and J.M. Zazula, ibidem, p. 100 (1994) * | |
95 | * * | |
96 | * [4] A. Ferrari and P.R. Sala, ibidem, p. 277 (1994). * | |
97 | * * | |
98 | * [5] A. Fasso', A. Ferrari, J. Ranft and P.R. Sala, "FLUKA: present * | |
99 | * status and future developments", presented at the IV Int. Conf. * | |
100 | * on Calorimetry in High Energy Physics, La Biodola (Elba), * | |
101 | * September 19-25 1993, Proceedings in press. * | |
102 | * * | |
103 | * [6] A. Fasso', A. Ferrari, J. Ranft, and P.R. Sala, "FLUKA: Perf- * | |
104 | * ormances and Applications in the Intermediate Energy Range", * | |
105 | * presented at the "Specialists' Meeting on Shielding Aspects of * | |
106 | * Accelerators, Targets & Irradiation Facilities", Arlington, * | |
107 | * April 28-29 1994, Proceedings in press. * | |
108 | * * | |
109 | *======================================================================* | |
110 | C. | |
111 | C. ------------------------------------------------------------------ | |
112 | C. | |
113 | C GHEISHA only if IHADR<3 (default) | |
114 | C | |
115 | CALL GHEISH | |
116 | C | |
117 | END |