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Featured researches published by R. Yokoyama.


Physical Review Letters | 2016

Candidate Resonant Tetraneutron State Populated by the He 4 (He 8, Be 8) Reaction

Keiichi Kisamori; S. Shimoura; Hiroyuki Miya; S. Michimasa; S. Ota; M. Assié; Hidetada Baba; Takahiro Baba; D. Beaumel; M. Dozono; T. Fujii; N. Fukuda; Shintaro Go; F. Hammache; E. Ideguchi; N. Inabe; Masatoshi Itoh; D. Kameda; S. Kawase; T. Kawabata; M. Kobayashi; Y. Kondo; Toshiyuki Kubo; Y. Kubota; M. Kurata-Nishimura; C. S. Lee; Y. Maeda; H. Matsubara; K. Miki; Takahiro Nishi

A candidate resonant tetraneutron state is found in the missing-mass spectrum obtained in the double-charge-exchange reaction ^{4}He(^{8}He,^{8}Be) at 186  MeV/u. The energy of the state is 0.83±0.65(stat)±1.25(syst)  MeV above the threshold of four-neutron decay with a significance level of 4.9σ. Utilizing the large positive Q value of the (^{8}He,^{8}Be) reaction, an almost recoilless condition of the four-neutron system was achieved so as to obtain a weakly interacting four-neutron system efficiently.


Physical Review Letters | 2017

94β -Decay Half-Lives of Neutron-Rich Cs55 to Ho67 : Experimental Feedback and Evaluation of the r -Process Rare-Earth Peak Formation

J. Wu; S. Nishimura; G. Lorusso; Peter Möller; E. Ideguchi; P. H. Regan; G. S. Simpson; P.-A. Söderström; P. M. Walker; Hiroshi Watanabe; Z. Y. Xu; H. Baba; F. Browne; R. Daido; P. Doornenbal; Y. F. Fang; G. Gey; T. Isobe; P. Lee; J. J. Liu; Z. Li; Z. Korkulu; Z. Patel; V. H. Phong; S. Rice; H. Sakurai; Laura C. Sinclair; T. Sumikama; M. Tanaka; A. Yagi

The β-decay half-lives of 94 neutron-rich nuclei ^{144-151}Cs, ^{146-154}Ba, ^{148-156}La, ^{150-158}Ce, ^{153-160}Pr, ^{156-162}Nd, ^{159-163}Pm, ^{160-166}Sm, ^{161-168}Eu, ^{165-170}Gd, ^{166-172}Tb, ^{169-173}Dy, ^{172-175}Ho, and two isomeric states ^{174m}Er, ^{172m}Dy were measured at the Radioactive Isotope Beam Factory, providing a new experimental basis to test theoretical models. Strikingly large drops of β-decay half-lives are observed at neutron-number N=97 for _{58}Ce, _{59}Pr, _{60}Nd, and _{62}Sm, and N=105 for _{63}Eu, _{64}Gd, _{65}Tb, and _{66}Dy. Features in the data mirror the interplay between pairing effects and microscopic structure. r-process network calculations performed for a range of mass models and astrophysical conditions show that the 57 half-lives measured for the first time play an important role in shaping the abundance pattern of rare-earth elements in the solar system.


Physical Review C | 2013

Collectivity evolution in the neutron-rich Pd isotopes toward the N=82 shell closure

He Wang; N. Aoi; Satoshi Takeuchi; Masafumi Matsushita; P. Doornenbal; Tohru Motobayashi; D. Steppenbeck; K. Yoneda; Hidetada Baba; L. Caceres; Zs. Dombrádi; K. Kobayashi; Y. Kondo; Jenny Lee; K. Li; H. L. Liu; Ryogo Minakata; D. Nishimura; Hideaki Otsu; S. Sakaguchi; H. Sakurai; Heiko Scheit; D. Sohler; Ye-Lei Sun; Zhengyang Tian; R. Tanaka; Y. Togano; Zs. Vajta; Zaihong Yang; Tetsuya Yamamoto

The neutron-rich, even-even 122,124,126Pd isotopes has been studied via in-beam gamma-ray spectroscopy at the RIKEN Radioactive Isotope Beam Factory. Excited states at 499(9), 590(11), and 686(17) keV were found in the three isotopes, which we assign to the respective 2+ -> 0+ decays. In addition, a candidate for the 4+ state at 1164(20) keV was observed in 122Pd. The resulting Ex(2+) systematics are essentially similar to those of the Xe (Z=54) isotopic chain and theoretical prediction by IBM-2, suggesting no serious shell quenching in the Pd isotopes in the vicinity of N=82.


ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2013: Proceedings of the 12th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG12) | 2014

β-decay of neutron-rich Z∼60 nuclei and the origin of rare earth elements

Jinguang Wu; S. Nishimura; G. Lorusso; Z.Y. Xu; H. Baba; F. Browne; R. Daido; P. Doornenbal; Y.F. Fang; E. Ideguchi; T. Isobe; Z. Li; Z. Patel; S. Rice; G. S. Simpson; L. Sinclair; P.-A. Söderström; T. Sumikama; Hiroshi Watanabe; A. Yagi; R. Yokoyama; N. Aoi; F. L. Bello Garrote; G. Benzoni; G. Gey; A. Gottardo; H. Nishibata; A. Odahara; H. Sakurai; M. Tanaka

A large fraction of the rare-earth elements observed in the solar system is produced in the astrophysical rapid neutron capture process (r-process). However, current stellar models cannot completely explain the relative abundance of these elements partially because of nuclear physics uncertainties. To address this problem, a β-decay spectroscopy experiment was performed at RI Beam Factory (RIBF) at RIKEN, aimed at studying a wide range of very neutron-rich nuclei with Z∼60 that are progenitors of the rare-earth elements with mass number A∼460. The experiment provides a test of nuclear models as well as experimental inputs for r-process calculations. This contribution presents the experimental setup and some preliminary results of the experiment.


Chinese Physics Letters | 2013

Observation of New Isotope 131Ag via the Two-Step Fragmentation Technique

Wang He; N. Aoi; S. Takeuchi; Masafumi Matsushita; P. Doornenbal; T. Motobayashi; D. Steppenbeck; K. Yoneda; K. Kobayashi; Jenny Lee; Liu Hong-Na; Y. Kondo; R. Yokoyama; H. Sakurai; Ye Yan-Lin

We report on the first observation of the neutron-rich nucleus 131Ag. This isotope was produced via fragmentation reactions of intense secondary radioactive ion beams, including 134,135Sn. The secondary beams were produced from induced fission reactions from a stable 238U beam at 345 MeV/nucleon. Secondary reaction residues were selected by the ZeroDegree spectrometer and identified by measuring their magnetic rigidity, time of flight, energy loss, and total kinetic energy.


Physical Review C | 2017

Nuclear structure and β -decay schemes for Te nuclides beyond N=82

B. Moon; C.-B. Moon; P.-A. Söderström; A. Odahara; R. Lozeva; B. Hong; F. Browne; H. S. Jung; P. Lee; C. S. Lee; A. Yagi; Cenxi Yuan; S. Nishimura; P. Doornenbal; G. Lorusso; T. Sumikama; Hiroshi Watanabe; I. Kojouharov; T. Isobe; H. Baba; H. Sakurai; R. Daido; Y. Fang; H. Nishibata; Z. Patel; S. Rice; L. Sinclair; Jinguang Wu; Z.Y. Xu; R. Yokoyama

We study for the first time the internal structure of 140Te through the beta-delayed gamma-ray spectroscopy of 140Sb. The very neutron-rich 140Sb, Z = 51 and N = 89, ions were produced by the in-flight fission of 238U beam on a 9Be target at 345 MeV per nucleon at the Radioactive Ion Beam Factory, RIKEN. The half-life and spin-parity of 140Sb are reported as 124(30) ms and (4-), respectively. In addition to the excited states of 140Te produced by the beta-decay branch, the beta-delayed one-neutron and two-neutron emission branches were also established. By identifying the first 2+ and 4+ excited states of 140Te, we found that Te isotopes persist their vibrator character with E(4+)/E(2+) = 2. We discuss the distinctive features manifest in this region, such as valence neutron symmetry and asymmetry, revealed in pairs of isotopes with the same neutron holes and particles with respect to N = 82.


Journal of the Physical Society of Japan | 2018

Identification of New Neutron-Rich Isotopes in the Rare-Earth Region Produced by 345 MeV/nucleon 238U

N. Fukuda; Toshiyuki Kubo; Daisuke Kameda; Naohito Inabe; Hiroshi Suzuki; Yohei Shimizu; Hiroyuki Takeda; Kensuke Kusaka; Y. Yanagisawa; M. Ohtake; K. Tanaka; Koichi Yoshida; Hiromi Sato; Hidetada Baba; M. Kurokawa; T. Ohnishi; N. Iwasa; Ayuko Chiba; Taku Yamada; E. Ideguchi; Shintaro Go; R. Yokoyama; T. Fujii; H. Nishibata; K. Ieki; D. Murai; S. Momota; Daiki Nishimura; Yoshiteru Sato; Jongwon Hwang

A search for new isotopes in the neutron-rich rare-earth region has been carried out using a 345 MeV/nucleon 238U beam at the RIKEN Nishina Center RI Beam Factory. Fragments produced were analyzed and identified using the BigRIPS in-flight separator. We observed a total of 29 new neutron-rich isotopes: 153Ba, 154,155,156La, 156,157,158Ce, 156,157,158,159,160,161Pr, 162,163Nd, 164,165Pm, 166,167Sm, 169Eu, 171Gd, 173,174Tb, 175,176Dy, 177,178Ho, and 179,180Er.


Physics Letters B | 2018

Is seniority a partial dynamic symmetry in the first ν g 9/2 shell?

A. I. Morales; G. Benzoni; H. Watanabe; G. de Angelis; S. Nishimura; L. Coraggio; A. Gargano; N. Itaco; T. Otsuka; Y. Tsunoda; P. Van Isacker; F. Browne; R. Daido; P. Doornenbal; Y. Fang; G. Lorusso; Z. Patel; S. Rice; L. Sinclair; P.-A. Söderström; T. Sumikama; J. J. Valiente-Dobón; J. Wu; Z.Y. Xu; A. Yagi; R. Yokoyama; H. Baba; R. Avigo; F. L. Bello Garrote; Nives Blasi

Abstract The low-lying structures of the midshell ν g 9 / 2 Ni isotopes 72Ni and 74Ni have been investigated at the RIBF facility in RIKEN within the EURICA collaboration. Previously unobserved low-lying states were accessed for the first time following β decay of the mother nuclei 72Co and 74Co. As a result, we provide a complete picture in terms of the seniority scheme up to the first ( 8 + ) levels for both nuclei. The experimental results are compared to shell-model calculations in order to define to what extent the seniority quantum number is preserved in the first neutron g 9 / 2 shell. We find that the disappearance of the seniority isomerism in the ( 8 1 + ) states can be explained by a lowering of the seniority-four ( 6 + ) levels as predicted years ago. For 74Ni, the internal de-excitation pattern of the newly observed ( 6 2 + ) state supports a restoration of the normal seniority ordering up to spin J = 4 . This property, unexplained by the shell-model calculations, is in agreement with a dominance of the single-particle spherical regime near 78Ni.


Proceedings of The 26th International Nuclear Physics Conference — PoS(INPC2016) | 2017

Sharaq Spectrometer: High-resolution Spectroscopy Using Exotic Beams And Reactions

S. Michimasa; S. Ota; M. Dozono; M. Takaki; Keiichi Kisamori; Hiroyuki Miya; M. Kobayashi; Yu Kiyokawa; Hidetada Baba; N. Fukuda; Naohito Inabe; S. Kawase; Toshiyuki Kubo; Y. Kubota; Cheong Soo Lee; Masafumi Matsushita; Hideyuki Sakai; A. Stolz; H. Tokieda; T. Uesaka; K. Yako; Y. Yanagisawa; R. Yokoyama; Koichi Yoshida; S. Shimoura

We introduce the recent development for increasing the performance of the SHARAQ spectrometer, which was operated at RI Beam Factory in RIKEN, Japan. The paper contains main achievements of our developments, which are detector developments, improvements of high-resolution performance at SHARAQ, and developments of new reaction probes to explore new kinds of nuclear responses. By using those new experimental technique, we recently performed various nuclear experiments at SHARAQ. We described here the preliminary results of the experiments together with their brief details.


Proceedings of the Conference on Advances in Radioactive Isotope Science (ARIS2014) | 2015

Heavy-Ion Double-Charge Exchange Study via a 12 C( 18 O, 18 Ne) 12 Be Reaction

M. Takaki; Hiroaki Matsubara; T. Uesaka; N. Aoi; M. Dozono; T. Hashimoto; T. Kawabata; S. Kawase; Keiichi Kisamori; Y. Kubota; Cheng Soo Lee; Jenny Lee; Y. Maeda; Shin’ichiro Michimasa; K. Miki; Shinsuke Ota; M. Sasano; S. Shimoura; T. Suzuki; K. Takahisa; Tsz Leung Tang; A. Tamii; H. Tokieda; K. Yako; R. Yokoyama; J. Zenihiro

Motonobu Takaki! (CNS, The University of Tokyo)! ! H. Matsubara2, T. Uesaka3, N. Aoi4, M. Dozono1, T. Hashimoto4, T. Kawabata5, 
 S. Kawase1, K. Kisamori1, Y. Kubota1, C.S. Lee1, J. Lee3, Y. Maeda6, S. Michimasa1,
 K. Miki4, S. Ota1, M. Sasano3, T. Suzuki4, K. Takahisa4, T.L. Tang1, A. Tamii4, 
 H. Tokieda1, K. Yako1, R. Yokoyama1, J. Zenihiro3, and S. Shimoura1! ! 1CNS, The University of Tokyo! 2National Institute of Radiological Science (NIRS)! 3RIKEN Nishina Center! 4Research Center for Nuclear Physics, Osaka University! 5Department of Physics, Kyoto University! 6Department of Applied Physics, University of Miyazaki

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P. Doornenbal

GSI Helmholtz Centre for Heavy Ion Research

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F. Browne

University of Brighton

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N. Aoi

University of Tokyo

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G. Lorusso

Michigan State University

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