Cálculo de la probabilidad de fotofisión de núcleos pesados en un rango de energía entre 0.1 GeV y 1.0 GeV

Abstract

This work has been made with the finality of calculate the distribution of photofission probability for heavy nuclei, which has been induced by real photons in an energy range between 0.1 GeV and 1.0 GeV, through the computational implementation of the intranunclear cascade model. In this model the process of fission is divided in two stages: intranuclear cascade and evaporative cascade. In the first stage, the incident photon starts a intranuclear cascade, in which some involved particles can escape from the nucleus leaving as a result a residual nucleus in a excited estate that is known as compound nucleus. the de-excitation of the compound nucleus is carried out in the second stage starting of different possible mechanism of evaporation´s particles and/ or fission.