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Stellar (n,gamma) cross section of 62Ni
Authors:Nassar H  Paul M  Ahmad I  Berkovits D  Bettan M  Collon P  Dababneh S  Ghelberg S  Greene J P  Heger A  Heil M  Henderson D J  Jiang C L  Käppeler F  Koivisto H  O'Brien S  Pardo R C  Patronis N  Pennington T  Plag R  Rehm K E  Reifarth R  Scott R  Sinha S  Tang X  Vondrasek R
Affiliation:Racah Institute of Physics, Hebrew University, Jerusalem, Israel, 91904.
Abstract:The 62Ni(n,gamma)63Ni(t(1/2)=100+/-2 yr) reaction plays an important role in the control of the flow path of the slow neutron-capture (s) nucleosynthesis process. We have measured for the first time the total cross section of this reaction for a quasi-Maxwellian (kT=25 keV) neutron flux. The measurement was performed by fast-neutron activation, combined with accelerator mass spectrometry to detect directly the 63Ni product nuclei. The experimental value of 28.4+/-2.8 mb, fairly consistent with a recent calculation, affects the calculated net yield of 62Ni itself and the whole distribution of nuclei with 62
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