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2016 Fiscal Year Final Research Report

Properties of low-to-medium neutron-rich neutron matter

Planned Research

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Project AreaNuclear matter in neutron stars investigated by experiments and astronomical observations
Project/Area Number 24105005
Research Category

Grant-in-Aid for Scientific Research on Innovative Areas (Research in a proposed research area)

Allocation TypeSingle-year Grants
Review Section Science and Engineering
Research InstitutionTokyo Institute of Technology

Principal Investigator

Nakamura Takashi  東京工業大学, 理学院, 教授 (50272456)

Co-Investigator(Kenkyū-buntansha) 下浦 享  東京大学, 理学(系)研究科(研究院), 教授 (10170995)
Co-Investigator(Renkei-kenkyūsha) Kondo Yosuke  東京工業大学, 理学院, 助教 (00455346)
Teranishi Takashi  九州大学, 理学研究院, 准教授 (10323495)
Research Collaborator Togano Yasuhiro  立教大学, 理学部, 助教
Kobayashi Nobuyuki  大阪大学, 核物理研究センター, 特任助教
Tostevin J. A.  Univ of Surrey, Professor
Hideaki Otsu  理化学研究所, 仁科加速器研究センター, チームリーダー
Project Period (FY) 2012-06-28 – 2017-03-31
Keywords実験核物理 / 不安定核 / 中性子星
Outline of Final Research Achievements

We have studied properties of very neutron-rich nuclear matter in order to elucidate the key properties of neutron star matter. (1)We have studied the pygmy dipole resonance in neutron-rich Ca isotopes using the newly constructed gamma-ray calorimeter. (2)We performed Coulomb breakup experiments of the two-neutron halo nuclei 19C and 19B, where enhanced electric dipole strengths are observed. This suggests dineutron correlation in these nuclei. We have found deformation-driven halo configuration for 31Ne and neighboring nuclei for the first time. (3) We have found evidence of the tetra-neutron state by the double charge exchange reaction. We have successfully measured precisely the mass of 26O, which was found barely unbound with respect to two-neutron emission. We have also successfully measured 28O for the first time. The nuclear interactions and many-body effects clarified by these experiments may shed light on the properties of neutron stars.

Free Research Field

実験核物理学

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Published: 2018-03-22  

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