• Open Access

Direct Determination of Fission-Barrier Heights Using Light-Ion Transfer in Inverse Kinematics

S. A. Bennett, K. Garrett, D. K. Sharp, S. J. Freeman, A. G. Smith, T. J. Wright, B. P. Kay, T. L. Tang, I. A. Tolstukhin, Y. Ayyad, J. Chen, P. J. Davies, A. Dolan, L. P. Gaffney, A. Heinz, C. R. Hoffman, C. Müller-Gatermann, R. D. Page, and G. L. Wilson
Phys. Rev. Lett. 130, 202501 – Published 19 May 2023
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Abstract

We demonstrate a new technique for obtaining fission data for nuclei away from β stability. These types of data are pertinent to the astrophysical r process, crucial to a complete understanding of the origin of the heavy elements, and for developing a predictive model of fission. These data are also important considerations for terrestrial applications related to power generation and safeguarding. Experimentally, such data are scarce due to the difficulties in producing the actinide targets of interest. The solenoidal-spectrometer technique, commonly used to study nucleon-transfer reactions in inverse kinematics, has been applied to the case of transfer-induced fission as a means to deduce the fission-barrier height, among other variables. The fission-barrier height of U239 has been determined via the U238(d,pf) reaction in inverse kinematics, the results of which are consistent with existing neutron-induced fission data indicating the validity of the technique.

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  • Received 17 November 2022
  • Revised 28 February 2023
  • Accepted 27 March 2023

DOI:https://doi.org/10.1103/PhysRevLett.130.202501

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

S. A. Bennett1, K. Garrett1, D. K. Sharp1,*, S. J. Freeman1,2, A. G. Smith1, T. J. Wright1, B. P. Kay3, T. L. Tang3,†, I. A. Tolstukhin3, Y. Ayyad4, J. Chen3, P. J. Davies5, A. Dolan6, L. P. Gaffney6, A. Heinz7, C. R. Hoffman3, C. Müller-Gatermann3, R. D. Page6, and G. L. Wilson8,3

  • 1Department of Physics and Astronomy, University of Manchester, Manchester M13 9PL, United Kingdom
  • 2CERN, CH-1211 Geneva 23, Switzerland
  • 3Physics Division, Argonne National Laboratory, Lemont, Illinois 60439, USA
  • 4IGFAE, Universidade de Santiago de Compostela, E-15782 Santiago de Compostela, Spain
  • 5School of Physics, Engineering and Technology, University of York, Heslington, York YO10 5DD, United Kingdom
  • 6Oliver Lodge Laboratory, University of Liverpool, Liverpool L69 7ZE, United Kingdom
  • 7Chalmers University of Technology, SE-41296 Göteborg, Sweden
  • 8Louisiana State University, Baton Rouge, Louisiana 70803, USA

  • *To whom all correspondence (inquiry) should be addressed. david.sharp@manchester.ac.uk
  • Present address: Department of Physics, Florida State University, Tallahassee, Florida 32306, USA.

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Issue

Vol. 130, Iss. 20 — 19 May 2023

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