出版社:SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要:The heavy neutron deficient p-nuclei are produced in explosive stellar environments via photodisintegration
reactions like (g ,n), (g ,p) and (g ,a) on r- or s- seed nuclei. The reaction rates of
p-nuclei are mostly based on theoretical parameterizations using statistical model calculations.
We study experimentally the photodisintegration rates of heavy nuclei at the bremsstrahlung facility
of the superconducting electron accelerator ELBE of FZ Dresden-Rossendorf. Photoactivation
measurements on the astrophysically relevant p-nuclei 92Mo and 144Sm have been performed
with bremsstrahlung end-point energies from 10.0 to 16.5 MeV. The activation yields are compared
with calculations using cross sections from recent Hauser-Feshbach models. The sensitivity
of the statistical models to the input ingredients like photon strength function, optical potentials
are tested against the experimental activation yield.