@article{3071999,
    title = "Cross-section measurements of radiative proton-capture reactions in Cd 112 at energies of astrophysical interest",
    author = "Psaltis, A. and Khaliel, A. and Assimakopoulou, E.-M. and Kanellakopoulos, A. and Lagaki, V. and Lykiardopoulou, M. and Malami, E. and Tsavalas, P. and Zyriliou, A. and Mertzimekis, T.J.",
    journal = "Physical Review C",
    year = "2019",
    volume = "99",
    number = "6",
    publisher = "American Physical Society",
    issn = "2469-9985, 2469-9993",
    doi = "10.1103/PhysRevC.99.065807",
    abstract = "Reactions involving the group of nuclei commonly known as p nuclei are part of the nucleosynthetic mechanisms at astrophysical sites. The In113 nucleus is such a case with several open questions regarding its origin at extreme stellar environments. In this paper, the experimental study of the cross sections of the radiative proton-capture reaction Cd112(p,γ)In113 is attempted for the first time at energies lying inside the Gamow window with an isotopically enriched Cd112 target. Two different techniques, the in-beam γ-ray spectroscopy and the activation method, have been applied. The latter method is required to account for the presence of a low-lying In113 isomer at 392 keV having a half-life of ≈100min. 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. © 2019 American Physical Society."
}