Abstract
Average continuum (Hauser-Feshbach) and resonance (Breit-Wigner) neutron capture rates for neutron-rich isotopes, determined on the basis of recent experimental nuclear physics input parameters, are compared to earlier theoretical reaction rates commonly used in astrophysical model computations.
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This work was supported by the Deutsche Forschungsgemeinschaft.
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Leist, B., Ziegert, W., Wiescher, M. et al. Neutron capture cross sections for neutron-rich isotopes. Z Physik A 322, 531–532 (1985). https://doi.org/10.1007/BF01412093
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DOI: https://doi.org/10.1007/BF01412093