* * $Id$ * * $Log$ * Revision 1.1.1.1 1995/10/24 10:20:41 cernlib * Geant * * #ifndef CERNLIB_GEANT321_PAREVT_INC #define CERNLIB_GEANT321_PAREVT_INC * * * parevt.inc * * * *=== parevt ===========================================================* * * *----------------------------------------------------------------------* * * * Created on 28-3-90 by A. Ferrari, INFN - Milan * * * * Last change on 20 april 1992 by Alfredo Ferrari * * * * included in: * * fluka * * bdnopt * * corevt * * distnu * * epilog * * eventv * * evevap * * evvini * * evxtes * * ferevv * * kaskad * * incini * * nucevv * * pmprab * * and in : * * prenuc * * umofin * * bimsel * * nucnuc * * nwisel * * pioabs * * prepre * * rstsel * * * * frdiff = fraction of the total number of events which are * * diffractive ones * * pthdff = momentum threshold for diffractive events * * diffractive ones * * fsprd0 = asymptotic reduction factor for cascade particle * * energy slope parameter * * fshpfn = modifying factor for bamjet momentum sharing jet * * function * * rn1gsc = correlation factor between shower and grey part- * * ticle multiplicities * * rn2gsc = correlation factor between shower and grey part- * * ticle multiplicities * * dpower = power exponent used in the binomial distributions * * for grey particles * * lpower = flag to signal if dpower is different from the * * default option (dpower=2) * * ldiffr = flag for particles undergoing diffractive events * * linctv = flag to switch on/off cascade nucleons and exci- * * tation energy (it is important for testing the * * generator * * levprt = flag for nuclear evaporation * * ldeexg = flag for nuclear deexcitation gammas * * lgdhpr = flag for geometry dependent calculations in the * * preequilibrium part * * lpreex = flag for explicit treatment of the first inte- * * ctions in the preequilibrium part * * lhlfix = flag for "freezing" the hole depth of the holes * * produced in the explicitly treated interactions * * in the preequilibrium part * * lprfix = flag for "freezing" the already sampled particle * * exciton energy in the preequilibrium part * * lparwv = flag to apply the Heisenberg principle according * * to the reduced DeBroglie wavelength in the calcu- * * lation of the impact parameter and in computing * * the particle position after interactions * * ilvmod = flag to select the level density option * * * *----------------------------------------------------------------------* * * * 30% of events, randomly choosen, are diffractive events!! * Now 20% (J. Ranft & A. Ferrari, 25-3-90) * PARAMETER ( FRDIFF = 0.2D+00 ) PARAMETER ( PTHDFF = 8.5D+00 ) PARAMETER ( ETHSEA = 1.0D+00 ) LOGICAL LDIFFR, LINCTV, LEVPRT, LHEAVY, LDEEXG, LGDHPR, LPREEX, & LHLFIX, LPRFIX, LPARWV, LPOWER COMMON / FKPARE / DPOWER, FSPRD0, FSHPFN, RN1GSC, RN2GSC, & LDIFFR (39), LPOWER, LINCTV, LEVPRT, LHEAVY, & LDEEXG, LGDHPR, LPREEX, LHLFIX, LPRFIX, LPARWV, & ILVMOD #endif