*$ CREATE SUMCOU.ADD *COPY SUMCOU * *=== Sumcou ===========================================================* * *----------------------------------------------------------------------* * * * All additions wrt the original one are: * * Copyright (C) 2005-2009 by Alfredo Ferrari & Paola Sala * * All Rights Reserved. * * * * * * SUMmary COUnters common for FLUKA9x/200x: * * * * (New version of the original STARS common) * * * * * * Created on 15 may 1990 by Alfredo Ferrari & Paola Sala * * Infn - Milan * * * * Last change on 23-mar-09 by Alfredo Ferrari * * * * * * Variable description: * * * * Ntstar = total number of stars generated (modulo 1000000000) * * Nestar = total number of elastic interactions generated * * (modulo 1000000000) * * Neulow = total number of low energy neutron interactions * * (modulo 1000000000) * * Numdec = total number of decays (modulo 1000000000) * * Numoph = total number of optical photons generated * * (modulo 1000000000) * * Mtstar = total number of stars generated / 100000000 * * Mestar = total number of elastic interactions generated * * / 1000000000 * * Meulow = total number of low energy neutron interactions * * / 1000000000 * * Mumdec = total number of decays / 1000000000 * * Mumoph = total number of optical photons generated /1000000000* * Wneulw(k,j) = total weight of the low energy neutron interactions * * Woptph(k,j) = total weight of generated optical photons * * Westar(k,j) = weight of the stars generated by * * different particle types * * Westop(k,j) = weight of particles of different types stopped * * Wedaug(k,j) = weight of the decay products * * Wekill(k,j) = weight of the time-killed particles * * Wedecy(k,j) = weight of the particles decayed * * Weifis(k,j) = weight of high energy fissions generated by particles* * of different kind * * Deccts(k,j) = decay c tau scoring * * Wdecct(k,j) = weight of the particles decayed for which a c tau * * scoring is done * * Weprdc(k,j) = weight of produced particles of different kind * * Wlwnsc(k,j) = weight of the low energy neutrons interaction secon- * * daries * * Wophsc(k,j) = weight of optical photons production/interaction * * secondaries * * Weipri = total weight of the primaries handled * * Westrs = total weight of the elastic interactions generated * * Edpsco(i,j) = energy deposition scoring (j = 1: prompt particles, * * j = 2: decay particles) * * Edpsco(1,j) = by ionisation * * Edpsco(2,j) = by pi-zeros and/or EM cascade * * Edpsco(3,j) = by nuclear excitation (or nuclear recoil * * and heavies if the evaporation module is * * activated) * * Edpsco(4,j) = by stopped particles * * Edpsco(5,j) = energy leaving the system * * Edpsco(6,j) = energy carried by discarded particles * * Edpsco(7,j) = by residual excitation energy (only if the * * evaporation module is activated) * * Edpsco(8,j) = by low energy neutrons (kerma due to low * * energy neutrons transport is in effect) * * Edpsco(9,j) = energy carried by time killed particles * * Edpsco(10,j)= energy wasted for nuclear binding energy * * effects for (low energy neutrons excluded) * * Edpsco(11,j)= energy wasted for nuclear binding energy * * effects for low energy neutrons * * * *----------------------------------------------------------------------* * COMMON / SUMCOU / WESTAR (-6:NALLWP,2), WESTOP (-6:NALLWP,2), & WEDAUG (-6:NALLWP,2), WEKILL (-6:NALLWP,2), & WEDECY (-6:NALLWP,2), WEIFIS (-6:NALLWP,2), & DECCTS (-6:NALLWP,2), WDECCT (-6:NALLWP,2), & WEPRDC (-6:NALLWP,2), WLWNSC (8,2), & WOPHSC (4,2), EDPSCO (11,2), WOPTPH, WNEULW, & WEIPRI, WESTRS, & NUMDEC, NTSTAR, NESTAR, NEULOW, NUMOPH, MUMDEC, & MTSTAR, MESTAR, MEULOW, MUMOPH SAVE / SUMCOU /