Abstract
The photodisintegration of the 32S nucleus is calculated in the framework of the microscopical model. The spread of the Fermi surface as well as particle and hole coupling with low-lying states are taken into account. The general features of the calculated absorption spectrum and different photonuclear reactions are discussed. An attempt is made to determine the origin of the peaks in the absorption spectrum on the basis of some reactions and calculated Coulomb form factors. Satisfactory agreement with experimental data is obtained.
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