Decay properties of 22Ne + α resonances and their impact on s-process nucleosynthesis

Decay properties of 22Ne + α resonances and their impact on s-process nucleosynthesis

The astrophysical s-process is one of the two main processes forming elements heavier than iron. A key outstanding uncertainty surrounding s-process nucleosynthesis is the neutron flux generated by the Ne22(α,n)25Mg reaction during the He-core and C-shell burning phases of massive stars. This reacti...

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Bibliografische gegevens
Hoofdauteurs: S. Ota, G. Christian, G. Lotay, W.N. Catford, E.A. Bennett, S. Dede, D.T. Doherty, S. Hallam, J. Hooker, C. Hunt, H. Jayatissa, A. Matta, M. Moukaddam, G.V. Rogachev, A. Saastamoinen, J.A. Tostevin, S. Upadhyayula, R. Wilkinson
Formaat: Artikel
Taal:English
Gepubliceerd in: Elsevier 2020-03-01
Reeks:Physics Letters B
Online toegang:http://www.sciencedirect.com/science/article/pii/S0370269320300605

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http://www.sciencedirect.com/science/article/pii/S0370269320300605

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