Resonance analysis of Sm147(n,α) cross sections: Comparison to optical model calculations and indications of nonstatistical effects

P. E. Koehler, Yu. M. Gledenov, T. Rauscher, and C. Fröhlich
Phys. Rev. C 69, 015803 – Published 30 January 2004

Abstract

We have measured the Sm147(n,α) cross section from 3eV to 500keV and performed an R-matrix analysis in the resolved region (En<700eV) to extract α widths for 104 resonances. We computed strength functions from these resonance parameters and compared them to transmission coefficients calculated using optical model potentials similar to those employed as inputs to statistical model calculations. The statistical model often is used to predict cross sections and astrophysical reaction rates. Comparing resonance parameters rather than cross sections allows more direct tests of potentials used in the model and hence should offer greater insight into possible improvements. In particular, an improved α+nucleus potential is needed for applications in nuclear astrophysics. In addition to providing a more direct test of the α+nucleus potential, the α-width distributions show indications of nonstatistical effects.

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  • Received 25 July 2003

DOI:https://doi.org/10.1103/PhysRevC.69.015803

©2004 American Physical Society

Authors & Affiliations

P. E. Koehler*

  • Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA

Yu. M. Gledenov

  • Joint Institute for Nuclear Research, Dubna, Russia

T. Rauscher and C. Fröhlich

  • Departement für Physik und Astronomie, Universität Basel, CH-4056 Basel, Switzerland

  • *Electronic address: koehlerpe@ornl.gov

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Vol. 69, Iss. 1 — January 2004

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