Towards a high-precision measurement of the 3He(α, γ)7Be cross section at LUNA

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The 2nd International Conference on Nuclear Physics in Astrophysics

Abstract

The 3He(4He, γ)7Be reaction is the key process for the production of 7Be and 8B neutrinos in the Sun. We have designed a new experimental setup to study this reaction with high accuracy at low energies using two different experimental techniques. The first method consists in measuring the prompt capture gamma-ray transitions with an ultra-low background germanium detector heavily shielded and placed at close distance from a 3He windowless gas target. With another fully shielded large-volume germanium detector we will also measure the β-decay of the 7Be residual nuclei. The aim of the experiment is to reduce the error on the astrophysical factor S3,4 to 4%.

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© 2006 Società Italiana di Fisica / Springer-Verlag

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Costantini, H. et al. (2006). Towards a high-precision measurement of the 3He(α, γ)7Be cross section at LUNA. In: Fülöp, Z., Gyürky, G., Somorjai, E. (eds) The 2nd International Conference on Nuclear Physics in Astrophysics. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-32843-2_26

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  • DOI: https://doi.org/10.1007/3-540-32843-2_26

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-32842-1

  • Online ISBN: 978-3-540-32843-8

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