2001
DOI: 10.1016/s0375-9474(00)00562-5
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Model calculations of the radiative capture process and the Brink–Axel hypothesis

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Cited by 7 publications
(3 citation statements)
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References 38 publications
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“…For the statistical calculations (the codes TALYS and EMPIRE contain as their essential parts the pre-equilibrium emission), the application of the models to reactions near the closed shells is not straightforward, and a special attention should be paid to different quantities, especially the level densities. This has been already demonstrated in our previous papers, where also a special care had to be applied for the reactions on double-closed 208 Pb [17,24]. For the DSD calculations, on the other hand, the doubleclosed nucleus is an advantage, as the single-particle states with well defined wave functions appear more clearly here.…”
Section: Gamma Spectra In Proton Radiative Capture Above 10 Mevmentioning
confidence: 62%
“…For the statistical calculations (the codes TALYS and EMPIRE contain as their essential parts the pre-equilibrium emission), the application of the models to reactions near the closed shells is not straightforward, and a special attention should be paid to different quantities, especially the level densities. This has been already demonstrated in our previous papers, where also a special care had to be applied for the reactions on double-closed 208 Pb [17,24]. For the DSD calculations, on the other hand, the doubleclosed nucleus is an advantage, as the single-particle states with well defined wave functions appear more clearly here.…”
Section: Gamma Spectra In Proton Radiative Capture Above 10 Mevmentioning
confidence: 62%
“…Here, deviations and even violations to the hypothesis are found [11,12]. However, for other theoretical applications, the assumption of the gBA hypothesis is successfully applied [13,14,15,16,17].…”
Section: Introductionmentioning
confidence: 99%
“…The study of excitation functions of both neutron-and proton-induced reactions [8,9,10,11] extended the applicability of the model to energies starting from few MeV to about 30 MeV. Significant improvement was the incorporation of spin into the formalism of the pre-equilibrium exciton model [12,13], which enabled also pre-equilibrium calculations leading to discrete states [14] and the comparison to the direct-semi-direct model calculations [3].…”
Section: Introductionmentioning
confidence: 99%