GCALOR consists of
The code has been The code is maintained by C. ZeitnitzUniversity of Wuppertal) and T.A. Gabriel (ORNL).
The two user subroutines GUPHAD and GUHADR have to be changed in order to retrieve the interaction probability (cross-section) of the current particle with the material it passed through.
SUBROUTINE GUPHAD
C get interaction probability
C CALL GPGHEI
C USE GCALOR INSTEAD OF GHEISHA
CALL CALSIG
RETURN
SUBROUTINE GUHADR
C inelastic hadronic interaction
C CALL GHEISH
C USE GCALOR INSTEAD OF GHEISHA
CALL GCALOR
RETURN
The GCALOR system is automatically initialized on first call. The initializations
consists of the following items:
News about the current version of GCALOR
Cesium cross-section (650kBytes compressed) file including (n,G) data from BNL-database. be aware, that this file has been thinned to 10% precision in order to get the size of the file down.
Cross-Section file 1 (474kBytes compressed) file contains ENDF/B-VI data for K-39 (natural composition), Mn-55, Sr-88, Sm-150 and Tb-159
Ge Cross-Section (546kBytes compressed) file contains Germanium data for the following isotopes: Ge-70, Ge-72, Ge-73, Ge-74, Ge-76
How to include the above files:
In addition to the GCALOR code and the data files, some CERN library routines and the GEANT library are needed to complete the simulation package