Cross section measurements of the 93Nb(p,γ)94Mo reaction at Ep=1.4-4.9 MeV relevant to the nucleosynthetic p process

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Radiative Capture, Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, 90<=A<=149, Abundances, Chemical Composition

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In-beam cross section measurements of the 93Nb(p,γ)94Mo reaction have been carried out at Ep=1.4-4.9 MeV, by using high efficiency high-purity Ge detectors, partly with BGO shields for Compton background suppression. From the resulting cross sections, which lie in the 0.5-300 μb range, astrophysical S factors as well as reaction rates have been obtained. By means of the statistical compound nucleus theory of Hauser and Feshbach, cross sections and reactions rates have also been calculated. A good agreement between the experimental data and the theoretical predictions has been found.

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