Nuclear level density and the determination of thermonuclear rates for astrophysics

@article{Rauscher1997NuclearLD,
  title={Nuclear level density and the determination of thermonuclear rates for astrophysics},
  author={Thomas Rauscher and F. Thielemann and Karl Ludwig Kratz},
  journal={Physical Review C},
  year={1997},
  volume={56},
  pages={1613-1625}
}
The prediction of cross sections for nuclei far off stability is crucial in the field of nuclear astrophysics. In recent calculations the nuclear level density{emdash}as an important ingredient to the statistical model (Hauser-Feshbach){emdash}has shown the highest uncertainties. We present a global parametrization of nuclear level densities within the back-shifted Fermi-gas formalism. Employment of an energy-dependent level density parameter a, based on microscopic corrections from a recent… 

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