Potential model for nuclear astrophysical fusion reactions with a square-well potential

@article{Ogura2019PotentialMF,
  title={Potential model for nuclear astrophysical fusion reactions with a square-well potential},
  author={Rei Ogura and Kouichi Hagino and Carlos A. Bertulani},
  journal={Physical Review C},
  year={2019}
}
The potential model for nuclear astrophysical reactions requires a considerably shallow nuclear potential when a square-well potential is employed to fit experimental data. We discuss the origin of this apparently different behavior from that obtained with a smooth Woods-Saxon potential, for which a deep potential is often employed. We argue that due to the sharp change of the potential at the boundary the radius parameter tends to be large in the square-well model, which results in a large… Expand
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