Probing Optimal Reaction Energy for Synthesis of Element 119 from 51V+248Cm Reaction with Quasielastic Barrier Distribution Measurement

Masaomi Tanaka, Pierre Brionnet, Miting Du, Julie Ezold, Kevin Felker, Benoît J.P. Gall, Shintaro Go, Robert K. Grzywacz, Hiromitsu Haba, Kouichi Hagino, Susan Hogle, Satoshi Ishizawa, Daiya Kaji, Sota Kimura, Thomas T. King, Yukiko Komori, Raiden K. Lemon, Milan G. Leonard, Kouji Morimoto, Kosuke MoritaDaisuke Nagae, Natsuki Naito, Toshitaka Niwase, Bertis C. Rasco, James B. Roberto, Krzysztof P. Rykaczewski, Satoshi Sakaguchi, Hideyuki Sakai, Yudai Shigekawa, Daniel W. Stracener, Shelley VanCleve, Yang Wang, Kouhei Washiyama, Takuya Yokokita

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Abstract

The quasielastic barrier distribution of 51V+248Cm was extracted by measuring the excitation function of quasielastic backscattering using a gas-filled recoil ion separator, GARIS-III. The obtained barrier distribution is well explained by the coupled-channels calculation, indicating a significant effect of the rotational excitation of deformed 248Cm. From the measured average Coulomb barrier height and deformation parameters of 248Cm, the side-collision energy leading to a compact configuration of colliding nuclei was obtained. The relation between the side collision energy and the excitation function of the evaporation-residue cross sections in the 48Ca248Cm system was evaluated as a reference for the 51V+248Cm case. The optimal reaction energy to synthesize a new element 119 at the 51V+248Cm fusion reaction (3n and 4n channels) was estimated with an aid of these experimental data.

Original languageEnglish
Article number084201
JournalJournal of the Physical Society of Japan
Volume91
Issue number8
DOIs
StatePublished - Aug 1 2022

Funding

Acknowledgments We would like to express our gratitude to the accelerator staff at RIKEN Nishina Center for providing 51V beam under the extremely stable operation and performing the quick change of the supplied beam energy during the entire machine time. The 248Cm isotope used in this research was supplied by the U.S. Department of Energy Isotope Program, managed by the Office of Isotope R&D and Production. The authors would like to thank Dr. T. Tanaka for the fruitful discussions on the interpretation of the data. The present work was supported in part by Grant-in-Aid for JSPS Research Fellow Grant No. 20J01229 and for JSPS KAKENHI Grant No. 20H01918. This work was partially supported by the U.S. DOE under the Contract No. DE-AC05-00OR22725.

FundersFunder number
U.S. Department of EnergyDE-AC05-00OR22725
Office of Isotope R and D and Production
Japan Society for the Promotion of Science20H01918, 20J01229

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