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In a realistic application of the SPA + RPA theory for calculation of the nuclear level densities we find that quantal fluctuation corrections (RPA) are important even up to temperature T=2.0 MeV. This leads to a good agreement between calculated numbers and the available experimental data for 104Pd and 114Sn, particularly the excitation energy (E∗) dependence. Furthermore, we also argue that a=S2/4E∗...
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