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Gamma-Ray Strength Functions

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Advances in Nuclear Physics

Abstract

The study of the energy dependence of multipole transition probabilities is a broad subject in which certain subfields have progressed much more rapidly than others. Thus for gamma rays ≲2 MeV, E1, M1, and E2 transition probabilities have been well studied (Per 66, SHR 66, SG 65), and at higher energies, ≳10 MeV, the absorption cross section and other properties of the E1 giant resonance are well known (Fir 70), but between these energies there are large gaps in our knowledge. In the present review we are concerned with the distribution of reduced radiation width, particularly for E1 and M1 radiation, in the less well-known “tail region” well below the peak of the E1 giant resonance. We will concentrate on elements with mass number A≳ 90, where a statistical description of radiative processes is appropriate, and on γ-ray energies above ~2 MeV.

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Authors and Affiliations

  1. Chalk River Nuclear Laboratories, Atomic Energy of Canada Limited, Chalk River, Canada

    G. A. Bartholomew, E. D. Earle, A. J. Ferguson, J. W. Knowles & M. A. Lone

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  1. G. A. Bartholomew
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  2. E. D. Earle
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  3. A. J. Ferguson
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  4. J. W. Knowles
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  5. M. A. Lone
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  1. Center for Theoretical Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts, USA

    Michel Baranger

  2. Department of Physics, University of British Columbia, Vancouver, B.C., Canada

    Erich Vogt

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Bartholomew, G.A., Earle, E.D., Ferguson, A.J., Knowles, J.W., Lone, M.A. (1973). Gamma-Ray Strength Functions. In: Baranger, M., Vogt, E. (eds) Advances in Nuclear Physics. Springer, Boston, MA. https://doi.org/10.1007/978-1-4615-9044-6_4

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