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

M. TanakaDepartment of Physics, Kyushu University, Fukuoka 819-0395, JapanP. BrionnetRIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, JapanMiting DuOak Ridge National Laboratory, Oak Ridge, TN 37831, U.S.AJulie EzoldOak Ridge National Laboratory, Oak Ridge, TN 37831, U.S.AKevin FelkerOak Ridge National Laboratory, Oak Ridge, TN 37831, U.S.AБ. ГаллUniversité de Strasbourg, CNRS, IPHC UMR 7178, 67037 Strasbourg, FranceS. GoDepartment of Physics, Kyushu University, Fukuoka 819-0395, JapanR. GrzywaczDepartment of Physics and Astronomy, University of Tennessee, Knoxville, TN 37996, U.S.AHiromitsu HabaRIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, JapanK. HaginoDepartment of Physics, Kyoto University, Kyoto 606-8502, JapanSusan HogleOak Ridge National Laboratory, Oak Ridge, TN 37831, U.S.ASatoshi IshizawaGraduate School of Science and Engineering, Yamagata University, Yamagata 990-8560, JapanD. KajiRIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, JapanSota KimuraRIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, JapanT. KingPhysics Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831, U.S.AYukiko KomoriRIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, JapanRaiden K. LemonDepartment of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University, Canberra, Australian Capital Territory 2601, AustraliaMilan G. LeonardDepartment of Nuclear Physics and Accelerator Applications, Research School of Physics, The Australian National University, Canberra, Australian Capital Territory 2601, AustraliaK. MorimotoRIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, JapanKosuke MoritaDepartment of Physics, Kyushu University, Fukuoka 819-0395, JapanD. NagaeDepartment of Physics, Kyushu University, Fukuoka 819-0395, JapanNatsuki NaitoGraduate School for Science, Kyushu University, Fukuoka 819-0395, JapanT. NiwaseDepartment of Physics, Kyushu University, Fukuoka 819-0395, JapanB. C. RascoPhysics Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831, U.S.AJ. B. RobertoPhysics Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831, U.S.AK. P. RykaczewskiPhysics Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831, U.S.AS. SakaguchiDepartment of Physics, Kyushu University, Fukuoka 819-0395, JapanH. SakaiRIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, JapanYudai ShigekawaRIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, JapanD. W. StracenerPhysics Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831, U.S.AShelley VanCleveOak Ridge National Laboratory, Oak Ridge, TN 37831, U.S.AYang WangRIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, JapanKouhei WashiyamaResearch Center for Superheavy Elements, Kyushu University, Fukuoka 819-0395, JapanTakuya YokokitaRIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan
2022en
ABI

Annotatsiya

Here, the quasielastic barrier distribution of <sup>51</sup>V+<sup>248</sup>Cm 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 <sup>248</sup>Cm. From the measured average Coulomb barrier height and deformation parameters of <sup>248</sup>Cm, 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 <sup>48</sup>Ca+<sup>248</sup>Cm system was evaluated as a reference for the <sup>51</sup>V+<sup>248</sup>Cm case. The optimal reaction energy to synthesize a new element 119 at the <sup>51</sup>V+<sup>248</sup>Cm fusion reaction (3n and 4n channels) was estimated with an aid of these experimental data.

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