Speaker
Leila Yettou
Description
In this study, the calculations of proton emission spectra produced by 58Ni(n,xp) reaction are used in the framework of preequilibrium models with the EMPIE and TALYS codes. Exciton model predictions combined with the Kalbach angular distribution syqtematics were used, and some necessary parameters have been investigated for our calculations. The comparison witj experimental data shows clear improvement over the Exciton model calculations.