²³Na(p,a)²⁰Ne

Marshall et al. 2023

Utilizing the high-resolution capabilities of the TUNL SPS, astrophysically important excited states in ²⁴Mg were populated via the (3He, d) transfer reaction. Astrophysically relevant states in 24Mg between 11 < E_x < 12 MeV were studied using high-resolution magnetic spectroscopy. In particular, careful calibration and compilation of previous results give a significantly lower resonance energy for the 133 keV resonance. These experimental data were then used to calculate the reaction rate.

Link to the paper.

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