Capture cross sections for the synthesis of new heavy nuclei using radioactive beams

  • A. Wakhle
  • , K. Hammerton
  • , Z. Kohley
  • , D. J. Morrissey
  • , K. Stiefel
  • , J. Yurkon
  • , J. Walshe
  • , K. J. Cook
  • , M. Dasgupta
  • , D. J. Hinde
  • , D. J. Jeung
  • , E. Prasad
  • , D. C. Rafferty
  • , C. Simenel
  • , E. C. Simpson
  • , K. Vo-Phuoc
  • , J. King
  • , W. Loveland
  • , R. Yanez

Research output: Contribution to journalArticlepeer-review

15 Scopus citations

Abstract

We have measured the capture-fission excitation functions for the reaction of stable K39 and radioactive K46 with Ta181 using the ReA3 facility at the National Superconducting Cyclotron Laboratory. In addition the capture-fission excitation function for the K39+Ta181 reaction was measured at Australian National University. The capture cross sections for the K46+Ta181 reaction are larger than those for the K39 induced reactions in the near barrier region although the reduced excitation functions for the two reactions do not indicate any fundamental differences between the reactions. The results of the measurements are compared to modern phenomenological models and microscopic time-dependent Hartree-Fock calculations. The implications of these measurements for the synthesis of heavy nuclei at radioactive beam facilities are discussed.

Original languageEnglish
Article number021602
JournalPhysical Review C
Volume97
Issue number2
DOIs
StatePublished - Feb 28 2018
Externally publishedYes

Funding

We gratefully acknowledge the efforts of A. Villari and the ReA3 staff for providing high quality beams of K 39 , 46 and for rapid changes of the beam energy during the experiment, some of which took only 15 min. We also acknowledge B. Swinton-Bland and K. Banerjee for checking analysis of the ANU data. We are especially grateful to N. Wang, and V. V. Sargsyan for performing calculations with their models for our reactions. This work was supported in part by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics under Grant No. DE-SC0014380 (OSU), Australian Research Council Grants No. FL110100098, No. FT120100760, No. DP140101337, No. DP160101254, and No. DP170102318 (ANU) and the National Science Foundation under Cooperative Agreement No. PHY-110251(MSU). We gratefully acknowledge NCRIS for support of operations of the ANU Heavy Ion Accelerator Facility. One of us (K.S.) wishes to acknowledge support from the U.S. DOE NNSA through the Nuclear Science and Security consortium under Grant No. DE-NA0003180. This work was supported in part by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics under Grant No. DE-SC0014380 (OSU), Australian Research Council Grants No. FL110100098, No. FT120100760, No. DP140101337, No. DP160101254, and No. DP170102318 (ANU) and the National Science Foundation under Cooperative Agreement No. PHY-110251(MSU). We gratefully acknowledge NCRIS for support of operations of the ANU Heavy Ion Accelerator Facility. One of us (K.S.) wishes to acknowledge support from the U.S. DOE NNSA through the Nuclear Science and Security consortium under Grant No. DE-NA0003180.

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