Abstract:Photoneutron cross sections were measured for 80 Se near the neutron separation energy with the laser Compton scattering γ rays. The stellar neutron capture rate for 79 Se was evaluated by using the photodisintegration data as constraints on the E1 γ strength function within the framework of the Hauser-Feshbach statistical model. The result is compared with the model calculation of Bao and Käppeler.
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