Measurements of the $$^{197}$$Au(n, $$\gamma $$) cross section up to 100 keV at the CSNS Back-n facility
Author:
Publisher
Springer Science and Business Media LLC
Subject
Nuclear Energy and Engineering,Nuclear and High Energy Physics
Link
https://link.springer.com/content/pdf/10.1007/s41365-021-00931-w.pdf
Reference38 articles.
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3. F. Käppeler, R. Gallino, S. Bisterzo et al., The $$s$$ process: nuclear physics, stellar models, and observations. Rev. Mod. Phys. 83, 157 (2011). https://doi.org/10.1103/RevModPhys.83.157
4. C. Lederer-Woods, U. Battino, P. Ferreira et al., Measurement of $$^{73}$$Ge($$n$$, $$\gamma $$) cross sections and implications for stellar nucleosynthesis. Phys. Lett. B 790, 458–465 (2019). https://doi.org/10.1016/j.physletb.2019.01.045
5. C. Massimi, C. Domingo-Pardo, G. Vannini et al., $$^{197}$$Au($$n$$, $$\gamma $$) cross section in the resonance region. Phys. Rev. C 81, 044616 (2010). https://doi.org/10.1103/PhysRevC.81.044616
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