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2018 Fiscal Year Final Research Report

Production and decay spectra of the neutron-rich hypernuclei and effects of channels coupling

Research Project

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Project/Area Number 16K05363
Research Category

Grant-in-Aid for Scientific Research (C)

Allocation TypeMulti-year Fund
Section一般
Research Field Particle/Nuclear/Cosmic ray/Astro physics
Research InstitutionOsaka Electro-Communication University

Principal Investigator

HARADA Toru  大阪電気通信大学, 共通教育機構, 教授 (70238187)

Co-Investigator(Kenkyū-buntansha) 平林 義治  北海道大学, 情報基盤センター, 准教授 (60271714)
Research Collaborator UMEYA Atsushi  
KOIKE Takahisa  
Project Period (FY) 2016-04-01 – 2019-03-31
Keywordsハイパー核 / ストレンジネス / チャネル結合 / 中性子過剰核 / 核反応 / 連続状態 / 少数多体系
Outline of Final Research Achievements

We study theoretically production and decay spectra of hypernuclei obtained at J-PARC facilities within a distorted-wave impulse approximation in order to see the effects and role of channel coupling between hypernucler states. The results are as follows: (1) A calculated spectra for a neutron-rich 6H_Lambda hypernucleus via the (pi-, K+) reaction on a 6Li target suggests that the Sigma-mixing probability amounts to about 0.3% via Sigma doorways in comparison with the experimental data. (2) A theoretical analysis shows that the Sigma-5He potential has a repulsive +30 MeV-strength in the real part. (3) Theoretical calculations of the 3He (pi, K) reaction including three-body break-up channels predict that the production cross section of the 3H_Lambda 1/2+ ground state is about 3 μb /sr.

Free Research Field

物理学,原子核理論,ストレンジネス核物理

Academic Significance and Societal Importance of the Research Achievements

ハイパー核研究の進展によって,宇宙の物質を構成している陽子や中性子の仲間であるバリオンや湯川粒子のパイ中間子などが担う核力全体の性質が解明され,宇宙にある中性子星やブラックホールの内部構造の理解につながると期待される。本研究でハイペロンと陽子・中性子間にはたらく2体核力やLambda NNなどの3体核力の性質についての理解が進み,核物質中でのハイペロンさらにはストレンジネスの役割とその重要性が分かってきたが,さらなる定量的な研究の進展が望まれる。

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Published: 2020-03-30  

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