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Pakou, A; Souliotis, G; Moustakidis, C (Ed.)In this work, we report the measurement of elastic and Coulomb break-up channels in6He+208Pb collisions at Elab= 19.3 MeV, close to the Coulomb barrier of this system ∼ 19 MeV. In the context of the astrophysical r-process, the reaction4He(2n,γ)6He has been proposed to be a key reaction in the path of synthesizing seed nuclei for the r-process, as12C, in an environment composed mainly of alpha particles and neutrons. Based on a theoretical approach for treating three body reactions by means of which its reaction rate can be inferred, our experimental approach aims to obtain an indirect measurement of the reaction rate of4He(2n,γ)6He by measuring the Coulomb breakup of6He under the intense electric field produced by a208Pb target nucleus. The experiment was carried out at the TriSol facility operated in the Nuclear Science Laboratory of the University of Notre Dame, USA, which delivered a6He beam together with other contaminants. Particular care must be taken for the alpha particles produced in the production reaction.more » « less
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Carmichael, Scott; O’Malley, Patrick; Bardayan, Daniel; Bailey, Thomas; Boomershine, Chevelle; Brodeur, Maxime; Coil, Sydney; Dembski, Cade; Gore, Tom; Jones, Chloe; et al (, EPJ Web of Conferences)Pakou, A; Souliotis, G; Moustakidis, C (Ed.)Nuclear reactions play a crucial role in determining the nucleosynthesis that occurs in astrophysical events. The rates of many reactions that significantly impact certain nucleosynthesis processes can not be currently measured via direct means. These reactions must be constrained in another manner, such as determining the level energies and other structure properties of the compound nuclei. In order to measure level energies of nuclei relevant to nuclear astrophysics, the Enge split-pole spectrograph has been installed and commissioned at the University of Notre Dame’s Nuclear Science Laboratory. The first scientific measurement has also been performed. Structure properties of58Cu were measured via the reaction58Ni(3He,t)58Cu to provide the first experimental constraint of the57Ni(p,γ)58Cu reaction rate, which impacts the production of of44Ti,57Fe, and59Ni in core-collapse supernovae. Preliminary analysis of this measurement confirms the level energies of states in58Cu that could lead to significant resonances in the57Ni(p,γ)58Cu reaction rate, while suggesting the presence of additional states that have not been previously observed but could also lead to significant resonances.more » « less
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