Large low-energy M1M1 strength for 56,57^{56,57}Fe within the nuclear shell model

preprint2014arXivOpen access

Abstract

A strong enhancement at low γγ-ray energies has recently been discovered in the γγ-ray strength function of 56,57^{56,57}Fe. In this work, we have for the first time obtained theoretical γγ decay spectra for states up to ≈8\approx 8 MeV in excitation for 56,57^{56,57}Fe. We find large B(M1)B(M1) values for low γγ-ray energies that provide an explanation for the experimental observations. The role of mixed E2E2 transitions for the low-energy enhancement is addressed theoretically for the first time, and it is found that they contribute a rather small fraction. Our calculations clearly show that the high-ℓ\ell (=f=f) diagonal terms are most important for the strong low-energy M1M1 transitions. As such types of 0ℏω0\hbarω transitions are expected for all nuclei, our results indicate that a low-energy M1M1 enhancement should be present throughout the nuclear chart. This could have far-reaching consequences for our understanding of the M1M1 strength function at high excitation energies, with profound implications for astrophysical reaction rates.

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