Strength of the $E_{\text{c.m.}} = 1113$ keV resonance in $^{20}$Ne$(p, \gamma)^{21}$Na

@article{Christian2013StrengthOT,
  title={Strength of the \$E\_\{\text\{c.m.\}\} = 1113\$ keV resonance in \$^\{20\}\$Ne\$(p, \gamma)^\{21\}\$Na},
  author={G. Christian and David Hutcheon and C. Akers and D. Connolly and J. Fallis and C. Ruiz},
  journal={Physical Review C},
  year={2013},
  volume={88},
  pages={038801}
}
The $^{20}$Ne$(p, \gamma)^{21}$Na reaction is the starting point of the NeNa cycle, which is an important process for the production of intermediate mass elements. The $E_{\text{cm}} = 1113$ keV resonance plays an important role in the determination of stellar rates for this reaction since it is used to normalize experimental direct capture yields at lower energies. The commonly accepted strength of this resonance, $\omega \gamma = 1.13 \pm 0.07$ eV, has been misinterpreted as the strength in… 

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