The reaction ${}^{14}\mathrm{N}(n,p){}^{14}\mathrm{C}$ is one of the main neutron poisons during $s$-process nucleosynthesis. In addition, the reaction provides insight into the yields of atmospheric nuclear weapon testing. Because of their high level of sensitivity, total neutron cross sections provide a great deal of constraint on the modeling of reaction cross sections through the $R$-matrix analyses used for nuclear data evaluations. Yet for ${}^{14}\mathrm{N}+n$ only one high sensitivity measurement is available, and it lacks detailed information about its experimental conditions and uncertainties. With these motivations in mind, a new measurement of the ${}^{14}\mathrm{N}+n$ total cross section was performed at the nELBE facility. The cross sections were found to be in good agreement with previous data over much of the energy range, with the key exception of the lowest energy resonance at a neutron energy of 433 keV.

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• Energy levels
• Hydrostatic stellar nucleosynthesis
• Nuclear astrophysics
• Resonance reactions
• 6 ≤ A ≤ 19
• Spin