Direct determination of radioactive nuclide production in astrophysical reactions by Accelerator Mass Spectrometry (AMS)

Physics – Nuclear Physics

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Transfer Reactions, Hydrostatic Stellar Nucleosynthesis, Charged-Particle Spectroscopy, 39<=A<=58

Scientific paper

We report on novel measurements of the total production cross section of long-lived nuclei produced in nuclear reactions relevant to astrophysical processes, using the Accelerator Mass spectrometry (AMS) technique at the Koffler accelerator of the Weizmann Institute as a direct ``atom-counting'' method. First results of these experiments for two such nuclides, 44Ti and 7Be, produced in nucleosynthesis sites and in solar fusion reactions, serve as a demonstration of the present approach and of its high sensitivity and very low background. The methodology and parameters of the present method, together with recent results, are presented. .

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