1997
DOI: 10.1016/s0370-2693(97)00662-x
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Many-body cascade calculation for photonuclear reactions

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Cited by 51 publications
(70 citation statements)
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“…Both intranuclear cascade and evaporation/fission calculations with the CRISP model have been extensively investigated yielding good results for reactions induced by photons, electrons and protons and observables such as neutron or proton multiplicity, fission and spallation cross sections, and fragment mass distributions [14,16,17,[22][23][24][25][26][27].…”
Section: Modelmentioning
confidence: 99%
“…Both intranuclear cascade and evaporation/fission calculations with the CRISP model have been extensively investigated yielding good results for reactions induced by photons, electrons and protons and observables such as neutron or proton multiplicity, fission and spallation cross sections, and fragment mass distributions [14,16,17,[22][23][24][25][26][27].…”
Section: Modelmentioning
confidence: 99%
“…During the time span of the binary scatterings, the remaining particles are supposed not to interact and the collisional term between the interacting particles inside the nuclear matter is approximated by the same quantity predicted for the vacuum. The basic concepts of the present calculation were first developed to study high-energy photonuclear reactions [3][4][5][6]. Although these versions have presented satisfactory results, they also had some inherent limitations related with the stochastic treatment of the Pauli-blocking mechanism and the incorporation of ambiguous quantities, such as stopping time parameters to determine the pre-equilibrium stage.…”
Section: A the Multicollisional Intranuclear Cascade Modelmentioning
confidence: 99%
“…This version was dedicated to the quasideuteron entrance channel and incorporates important improvements, most of them related with a nonstochastic treatment for the Pauli-blocking mechanism, in comparison with previous approaches [3][4][5][6]. Neutron multiplicities and the total photoabsorption cross sections for Sn, Ce, Ta, and Pb were consistently described using the MCMC model to describe the rapid stage of the nuclear reaction plus an evaporation Monte Carlo routine, based on the Weisskopf statistical theory, to address the de-excitation of the compound nucleus (CN) in terms of the competition between particle evaporation and nuclear fission.…”
Section: Introductionmentioning
confidence: 99%
“…CRISP is a Monte Carlo code for simulating nuclear reactions [20] that uses a two step process. First, an intranuclear cascade is simulated following a time-ordered sequence of collisions in a many-body system [21,22], and when the intranuclear cascade is finished the evaporation of nucleons and alpha-particles starts in competition with fission [23].…”
Section: Introductionmentioning
confidence: 99%
“…In the simulation, reactions can be initiated by intermediate and high energy protons [22] or photons [24][25][26]. It has been extended to energies up to 3.5 GeV [27], and it was shown that the CRISP code can give good results for total photonuclear absorption cross sections from approximately 50 MeV, where the quasi-deuteron absorption mechanism is dominant, up to 3.5 GeV, where the socalled photon-hadronization mechanism is dominant, leading to a shadowing effect in the cross section [27].…”
Section: Introductionmentioning
confidence: 99%