Examination of the low-energy enhancement of the γ-ray strength function of Fe56

M. D. Jones et al.
Phys. Rev. C 97, 024327 – Published 22 February 2018

Abstract

A model-independent technique was used to determine the γ-ray strength function (γSF) of Fe56 down to γ-ray energies less than 1 MeV for the first time with GRETINA using the (p,p) reaction at 16 MeV. No difference was observed in the energy dependence of the γSF built on 2+ and 4+ final states, supporting the Brink hypothesis. In addition, angular distribution and polarization measurements were performed. The angular distributions are consistent with dipole radiation. The polarization results show a small bias towards magnetic character in the region of the enhancement.

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  • Received 13 November 2017

DOI:https://doi.org/10.1103/PhysRevC.97.024327

©2018 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

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Vol. 97, Iss. 2 — February 2018

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