Consistency of photon strength function models with data from the Mo94(d,pγγ) reaction

M. Krtička, M. Wiedeking, F. Bečvář, and S. Valenta
Phys. Rev. C 93, 054311 – Published 9 May 2016

Abstract

Recently published study on the γ-ray energy dependence of photon strength functions (PSFs) from the population of Mo95 low-lying levels in the Mo94(d,pγγ)Mo95 reaction set out to answer some important questions related to the PSFs below the neutron separation energy in the Mo region. In this paper we discuss in detail actual relations of the quantities measured in this reaction to the PSFs and check the consistency of several available PSF models with experimental data. A broad variety of models was found to be consistent with experimental data at low Eγ. Although the photon strength very likely increases with decreasing energy at Eγ3 MeV, the data are unable to clearly differentiate whether the decrease follows the shape proposed from Oslo-type experiments or predictions of the generalized Lorentzian E1 model. The PSF shape at energies of 57 MeV is steeper than predicted by any standard model.

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  • Received 15 March 2016

DOI:https://doi.org/10.1103/PhysRevC.93.054311

©2016 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

M. Krtička1, M. Wiedeking2, F. Bečvář1, and S. Valenta1

  • 1Faculty of Mathematics and Physics, Charles University, V Holešovičkách 2, Prague 8, Czech Republic
  • 2iThemba LABS, P.O. Box 722, 7129 Somerset West, South Africa

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Issue

Vol. 93, Iss. 5 — May 2016

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