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Reactions involving the group of nuclei commonly known as p nuclei are partof the nucleosynthetic mechanisms at astrophysical sites. The $^{113}$Innucleus is such a case with several open questions regarding its origin atextreme stellar environments. In this work, the experimental study of the crosssections of the radiative proton-capture reaction$^{112}$Cd(p,$\gamma$)$^{113}$In is attempted for the first time at energieslying inside the Gamow window with an isotopically enriched $^{112}$Cd target.Two different techniques, the in-beam $\gamma$-ray spectroscopy and theactivation method, have been applied. The latter method is required to accountfor the presence of a low-lying $^{113}$In isomer at 392 keV having a halflifeof $\approx 100$ min. From the cross sections, the astrophysical S factors andthe isomeric ratios have been additionally deduced. The experimental resultsare compared to detailed Hauser-Feshbach theoretical calculations using TALYS,and discussed in terms of their significance to the optical model potentialinvolved.

Cross-section measurements of radiative proton-capture reactions in $^{112}$Cd at energies of astrophysical interest