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

R. Ogura, K. Hagino, and C. A. Bertulani
Phys. Rev. C 99, 065808 – Published 25 June 2019

Abstract

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 absorption radius. The wave function then needs to be suppressed in the absorption region, which can eventually be achieved by using a shallow potential. We thus clarify the reason why the square-well potential has been able to reproduce a large amount of fusion data.

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  • Received 12 March 2019

DOI:https://doi.org/10.1103/PhysRevC.99.065808

©2019 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

R. Ogura1, K. Hagino1,2, and C. A. Bertulani3

  • 1Department of Physics, Tohoku University, Sendai 980-8578, Japan
  • 2Research Center for Electron Photon Science, Tohoku University, 1-2-1 Mikamine, Sendai 982-0826, Japan
  • 3Department of Physics and Astronomy, Texas A&M University-Commerce, Commerce, Texas 75429-3011, USA

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Issue

Vol. 99, Iss. 6 — June 2019

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