Investigation of the 23Na (p,γ) 24Mg and 23Na (p,α) 20Ne reactions via ( 3He ,d) spectroscopy

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Hydrostatic Stellar Nucleosynthesis, Nuclear Reactions Involving Few-Nucleon Systems, Transfer Reactions, Origin, Formation, And Abundances Of The Elements

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States near the 23Na +p threshold in 24Mg were investigated using the 23Na ( 3He ,d) 24Mg reaction over the angular range of 5°⩽ θlab ⩽35° at E ( 3He ) =20 MeV . Spectroscopic factors were extracted for states corresponding to resonances in the 23Na (p,γ) 24Mg and 23Na (p,α) 20Ne reactions. We find that one state, corresponding to a previously unobserved resonance at Ec.m. =138 keV , may make a significant contribution to the rates of both reactions at low temperatures. Another state, corresponding to a possible resonance at Ec.m. =37 keV may make a small contribution to the 23Na (p,α) 20Ne reaction. New rates for the 23Na (p,γ) 24Mg and 23Na (p,α) 20Ne reactions are presented and the astrophysical implications are discussed.

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