Cross-section measurements of radiative proton-capture reactions in Cd at energies of astrophysical interest
A. Psaltis🇨🇦 · A. Khaliel · E.-M. Assimakopoulou · A. Kanellakopoulos🇧🇪 · V. Lagaki🇨🇭 · M. Lykiardopoulou🇨🇦 · E. Malami🇳🇱 · P. Tsavalas · A. Zyriliou · T. J. Mertzimekis🇬🇷
Reactions involving the group of nuclei commonly known as p nuclei are part of the nucleosynthetic mechanisms at astrophysical sites. The In nucleus is such a case with several open questions regarding its origin at extreme stellar environments. In this work, the experimental study of the cross sections of the radiative proton-capture reaction Cd(p,)In is attempted for the first time at energies lying inside the Gamow window with an isotopically enriched Cd target. Two different techniques, the in-beam -ray spectroscopy and the activation method, have been applied. The latter method is required to account for the presence of a low-lying In isomer at 392 keV having a halflife of min. From the cross sections, the astrophysical S factors and the isomeric ratios have been additionally deduced. The experimental results are compared to detailed Hauser-Feshbach theoretical calculations using TALYS, and discussed in terms of their significance to the optical model potential involved.