Direct total cross section measurement of the 16O(α,γ)20Ne reaction at Ec.m.=2.26 MeV

Details Direct total cross section measurement of the 16O(α,γ)20Ne reaction at Ec.m.=2.26 MeV Direct total cross section measurement of the 16O(α,γ)20Ne reaction at Ec.m.=2.26 MeV

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011phrvc..84b2801h&link_type=abstract

Physical Review C, vol. 84, Issue 2, id. 022801

Physics

Stellar Helium Burning, Origin, Formation, And Abundances Of The Elements, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages

Scientific paper

In stellar helium burning, 16O represents the endpoint of the helium-burning sequence due to the low rate of 16O(α,γ)20Ne. We present a new direct measurement of the total capture reaction rate of 16O(α,γ)20Ne at Ec.m.=2.26MeV employing the DRAGON recoil separator. For the first time, the total S factor and its contributing direct capture transitions could be determined in one experiment.

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