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Decay spectroscopy of neutron-rich nuclei produced in multinucleon transfer reactions at KISS

ORAL · Invited

Abstract

Multinucleon transfer (MNT) reactions have gained renewed interest in recent years as they provide a pathway to access neutron-rich nuclei that are difficult to produce by other methods such as complete fusion and fragmentation [1]. Because MNT reactions produce a wide variety of nuclides around both the projectile and target nuclei with wide angular and energy distributions, the development of experimental techniques to collect, separate, and identify the reaction products of interest is essential to perform their decay spectroscopy. In particular, exotic nuclei that are far from the projectile or target nuclei are produced very infrequently and may be buried among more abundant reaction products. Furthermore, for short-lived nuclei with lifetimes of less than a few minutes, rapid isolation becomes critical.

We are developing the KEK Isotope Separation System (KISS) focusing on the extraction of MNT reaction products at the RIBF facility of the RIKEN Nishina Center [2]. This is an argon-gas-cell-based laser ion source coupled with an isotope separation online system. All reaction products are efficiently collected and neutralized by argon gas, and nuclides of interest are element-selectively ionized by laser resonance method to be accelerated and mass-separated with a bipolar electromagnet for their high-purity decay spectroscopy. We have performed decay spectroscopy of neutron-rich nuclei of refractory elements near the N = 126 region. Recently, we extracted the neutron-rich actinide nuclei produced by MNT reactions with 238U beams to extend our spectroscopic studies to the neutron-rich actinide region.

In this presentation, we will report the experimental methods and results of KISS, including the perspective of decay spectroscopy on the upgrade plan KISS-II.



References

[1] Y.X. Watanabe et al., Phys. Rev. Lett. 115, 172503 (2015).

[2] Y. Hirayama et al., Nucl. Instrum. Meth. B 353, 4 (2015).

Publication: T. Niwase et al., Phys. Rev. Lett. 130, 132502 (2023).<br>Y. Hirayama et al., Phys. Rev. C 106, 034326 (2022).<br>M. Mukai et al., Phys. Rev. C 105, 034331 (2022).<br>Y.X. Watanabe et al., Phys. Rev. C 104, 024330 (2021).<br>M. Ahmed et al., Phys. Rev. C 103, 054312 (2021).<br>Y.X. Watanabe et al., Phys. Rev. C 103, 019902(E) (2021).<br>Y.X. Watanabe et al., Phys. Rev. C 101, 041305(R) (2020).<br>H. Watanabe et al., Phys. Lett. B 814, 136088 (2021).<br>P.M. Walker et al., Phys. Rev. Lett. 125, 192505 (2020).<br>M. Mukai et al., Phys. Rev. C 102, 054307 (2020).<br>H. Choi et al., Phys. Rev. C 102, 034309 (2020).<br>Y. Hirayama et al., Phys. Rev. C 98, 014321 (2018).<br>Y. Hirayama et al., Nucl. Instrum. and Methods A 997, 165152 (2021).<br>M. Mukai et al., Nucl. Instrum. and Methods A 884, 1 – 10 (2018).<br>Y. Hirayama et al., Phys. Rev. C 96, 014307 (2017).<br>Y. Hirayama et al., Nucl. Instrum. and Methods B 412, 11 – 18 (2017).<br>Y. Hirayama et al., Nucl. Instrum. and Methods B 353, 4 – 15 (2015).

Presenters

  • Yutaka X Watanabe

    KEK Wako Nuclear Science Center, KEK, High Energy Accelerator Research Organization (KEK), WNSC, IPNS, High Energy Accelerator Research Organization (KEK), Wako Nuclear Science Center (WNSC), KEK, Japan, WNSC, KEK, Wako Nuclear Science Center (WNSC), KEK

Authors

  • Yutaka X Watanabe

    KEK Wako Nuclear Science Center, KEK, High Energy Accelerator Research Organization (KEK), WNSC, IPNS, High Energy Accelerator Research Organization (KEK), Wako Nuclear Science Center (WNSC), KEK, Japan, WNSC, KEK, Wako Nuclear Science Center (WNSC), KEK

  • Yoshikazu Hirayama

    KEK Wako Nuclear Science Center, KEK, High Energy Accelerator Research Organization (KEK), WNSC, IPNS, High Energy Accelerator Research Organization (KEK), WNSC, KEK, Wako Nuclear Science Center (WNSC), KEK

  • Momo Mukai

    Nagoya University, Department of Physics, Nagoya University, Japan, RNC, RIKEN

  • Toshitaka Niwase

    KEK Wako Nuclear Science Center, High Energy Accelerator Research Organization (KEK), WNSC, IPNS, High Energy Accelerator Research Organization (KEK), KEK, Wako Nuclear Science Center (WNSC), KEK, Japan, Wako Nuclear Science Center (WNSC), KEK

  • Peter Schury

    High Energy Accelerator Research Organization (KEK), WNSC, IPNS, High Energy Accelerator Research Organization (KEK), Wako Nuclear Science Center (WNSC), KEK, Japan, WNSC, KEK, Wako Nuclear Science Center (WNSC), KEK, KEK Wako Nuclear Science Center

  • Marco Rosenbusch

    RIKEN Nishina Center, RIKEN Nishina Center for Accelerator-Based Science, RIKEN Nishina Center for Accelerator-Based Science, Japan, WNSC, KEK

  • Sota Kimura

    KEK Wako Nuclear Science Center, WNSC, IPNS, High Energy Accelerator Research Organization (KEK), Wako Nuclear Science Center (WNSC), KEK, Japan

  • Hironobu Ishiyama

    RIKEN Nishina Center, RIKEN Nishina Center for Accelerator-Based Science, RIKEN Nishina Center for Accelerator-Based Science, Japan, RNC, RIEKN

  • Sunchan Jeong

    WNSC, IPNS, High Energy Accelerator Research Organization (KEK), KEK, WNSC, KEK

  • Hiroari Miyatake

    High Energy Accelerator Research Organization (KEK), WNSC, IPNS, High Energy Accelerator Research Organization (KEK), KEK, WNSC, KEK

  • Michiharu Wada

    KEK Wako Nuclear Science Center, High Energy Accelerator Research Organization (KEK), KEK, WNSC, IPNS, High Energy Accelerator Research Organization (KEK), Wako Nuclear Science Center (WNSC), KEK, Japan, WNSC, KEK, Wako Nuclear Science Center (WNSC), KEK

  • Shun Iimura

    Department of Physics, College of Science, Rikkyo University, Rikkyo University, RNC, RIKEN, Department of Physics, Rikkyo University

  • Akihiro Taniguchi

    Institute for Integrated Radiation and Nuclear Science, Kyoto University, KURNS, Kyoto University