Photo-fission Cross Section of Uranium Isotopes using three humps barrier

In this investigation calculated cross section of induced photo-fission of uranium Isotopes, 230-239U using simulation through optical model are compared with experimental data. To obtain photo-fission cross section transition probability through three humps fission barrier is used. Also, to calculate level density of compound nucleus, improved version of Enhanced Generalized Super-fluid Model (EGSM) is employed. Simulated cross sections using Empire code for these Isotopes in a wide range of energy are compared with available experimental data. Cross sections for different isotopes of uranium as a function of energy in the range 5 to 20 MeV are plotted. Good agreement achieved when the results of Empire code are compared with available experimental data.