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Low-energy enhancement in the magnetic dipole radiation of actinide nuclei

C. Rodgers, D. DeMartini, Y. Alhassid

Abstract

We present the first theoretical results of the magnetic dipole (M1) $γ$-ray strength function ($γ$SF) for actinide nuclei within the shell-model Monte Carlo (SMMC) method. We observe a low-energy enhancement (LEE) in the M1 $γ$SFs of the six nuclei studied here, which serves as the first evidence, theoretical or experimental, that the LEE persists in the actinides. We also identify a scissors mode resonance in all six nuclei, which we compare with recent Oslo-method experiments.

Low-energy enhancement in the magnetic dipole radiation of actinide nuclei

Abstract

We present the first theoretical results of the magnetic dipole (M1) -ray strength function (SF) for actinide nuclei within the shell-model Monte Carlo (SMMC) method. We observe a low-energy enhancement (LEE) in the M1 SFs of the six nuclei studied here, which serves as the first evidence, theoretical or experimental, that the LEE persists in the actinides. We also identify a scissors mode resonance in all six nuclei, which we compare with recent Oslo-method experiments.

Paper Structure

This paper contains 13 equations, 3 figures, 2 tables.

Figures (3)

  • Figure 1: The M1 strength functions $S_{M1}$ for the actinides at temperatures near the neutron separation energy. The blue solid lines are the SMMC+MEM results with shaded blue bands representing the uncertainties, and the red dashed lines are the SPA priors.
  • Figure 2: The de-excitation strength functions $f_{M1}$ (\ref{['eq:fm1_2']}) of the actinides calculated near the neutron separation energies. The blue solid lines are the SMMC+MEM results with shaded blue bands representing the uncertainties, and the red dashed lines are the SPA priors.
  • Figure 3: The slope parameter $\kappa$, obtained by fitting the LEE to Eq. \ref{['eq:LEE_fit']}, as a function of the initial energy for all six nuclei.