• 文献检索
  • 文档翻译
  • 深度研究
  • 学术资讯
  • Suppr Zotero 插件Zotero 插件
  • 邀请有礼
  • 套餐&价格
  • 历史记录
应用&插件
Suppr Zotero 插件Zotero 插件浏览器插件Mac 客户端Windows 客户端微信小程序
定价
高级版会员购买积分包购买API积分包
服务
文献检索文档翻译深度研究API 文档MCP 服务
关于我们
关于 Suppr公司介绍联系我们用户协议隐私条款
关注我们

Suppr 超能文献

核心技术专利:CN118964589B侵权必究
粤ICP备2023148730 号-1Suppr @ 2026

文献检索

告别复杂PubMed语法,用中文像聊天一样搜索,搜遍4000万医学文献。AI智能推荐,让科研检索更轻松。

立即免费搜索

文件翻译

保留排版,准确专业,支持PDF/Word/PPT等文件格式,支持 12+语言互译。

免费翻译文档

深度研究

AI帮你快速写综述,25分钟生成高质量综述,智能提取关键信息,辅助科研写作。

立即免费体验

观测到一个关联的自由四核子系统。

Observation of a correlated free four-neutron system.

机构信息

Technische Universität Darmstadt, Fachbereich Physik, Darmstadt, Germany.

GSI Helmholtzzentrum für Schwerionenforschung GmbH, Darmstadt, Germany.

出版信息

Nature. 2022 Jun;606(7915):678-682. doi: 10.1038/s41586-022-04827-6. Epub 2022 Jun 22.

DOI:10.1038/s41586-022-04827-6
PMID:35732764
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC9217746/
Abstract

A long-standing question in nuclear physics is whether chargeless nuclear systems can exist. To our knowledge, only neutron stars represent near-pure neutron systems, where neutrons are squeezed together by the gravitational force to very high densities. The experimental search for isolated multi-neutron systems has been an ongoing quest for several decades, with a particular focus on the four-neutron system called the tetraneutron, resulting in only a few indications of its existence so far, leaving the tetraneutron an elusive nuclear system for six decades. Here we report on the observation of a resonance-like structure near threshold in the four-neutron system that is consistent with a quasi-bound tetraneutron state existing for a very short time. The measured energy and width of this state provide a key benchmark for our understanding of the nuclear force. The use of an experimental approach based on a knockout reaction at large momentum transfer with a radioactive high-energy He beam was key.

摘要

长期以来,核物理学界一直存在一个问题,即不带电荷的核系统是否能够存在。据我们所知,只有中子星代表了近乎纯中子的系统,其中中子在引力的作用下被挤压到极高的密度。几十年来,人们一直在实验上寻找孤立的多中子系统,特别是寻找被称为四中子的四中子系统,目前为止只有少数几个存在的迹象,这使得四中子成为了一个难以捉摸的核系统长达六十年。在这里,我们报告了在四中子系统中在阈附近观察到的类似于共振的结构,这与存在极短时间的准束缚四中子态一致。该态的测量能量和宽度为我们理解核力提供了一个关键的基准。使用基于放射性高能氦束在大动量转移下的 knockout 反应的实验方法是关键。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/fae372b31d3f/41586_2022_4827_Fig12_ESM.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/5710776f8aec/41586_2022_4827_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/8a0e844fa650/41586_2022_4827_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/4adefecb3ee6/41586_2022_4827_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/734f58b2ce99/41586_2022_4827_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/6f8cb2107569/41586_2022_4827_Fig5_ESM.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/2305ba68079d/41586_2022_4827_Fig6_ESM.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/c1e13234b9ec/41586_2022_4827_Fig7_ESM.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/7293ef390278/41586_2022_4827_Fig8_ESM.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/a54462e277d1/41586_2022_4827_Fig9_ESM.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/4a85b77d29cb/41586_2022_4827_Fig10_ESM.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/0ed6a38c6454/41586_2022_4827_Fig11_ESM.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/fae372b31d3f/41586_2022_4827_Fig12_ESM.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/5710776f8aec/41586_2022_4827_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/8a0e844fa650/41586_2022_4827_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/4adefecb3ee6/41586_2022_4827_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/734f58b2ce99/41586_2022_4827_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/6f8cb2107569/41586_2022_4827_Fig5_ESM.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/2305ba68079d/41586_2022_4827_Fig6_ESM.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/c1e13234b9ec/41586_2022_4827_Fig7_ESM.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/7293ef390278/41586_2022_4827_Fig8_ESM.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/a54462e277d1/41586_2022_4827_Fig9_ESM.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/4a85b77d29cb/41586_2022_4827_Fig10_ESM.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/0ed6a38c6454/41586_2022_4827_Fig11_ESM.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a59a/9217746/fae372b31d3f/41586_2022_4827_Fig12_ESM.jpg

相似文献

1
Observation of a correlated free four-neutron system.观测到一个关联的自由四核子系统。
Nature. 2022 Jun;606(7915):678-682. doi: 10.1038/s41586-022-04827-6. Epub 2022 Jun 22.
2
From hadrons to quarks in neutron stars: a review.从强子到中子星中的夸克:综述。
Rep Prog Phys. 2018 May;81(5):056902. doi: 10.1088/1361-6633/aaae14. Epub 2018 Feb 9.
3
Can Tetraneutron be a Narrow Resonance?四中子能成为窄共振态吗?
Phys Rev Lett. 2017 Jul 21;119(3):032501. doi: 10.1103/PhysRevLett.119.032501.
4
Nuclear physics. Momentum sharing in imbalanced Fermi systems.核物理。非对称费米体系中的动量分配。
Science. 2014 Oct 31;346(6209):614-7. doi: 10.1126/science.1256785. Epub 2014 Oct 16.
5
Candidate Resonant Tetraneutron State Populated by the ^{4}He(^{8}He,^{8}Be) Reaction.通过\(^{4}He(^{8}He,^{8}Be)\)反应产生的候选共振四中子态
Phys Rev Lett. 2016 Feb 5;116(5):052501. doi: 10.1103/PhysRevLett.116.052501. Epub 2016 Feb 3.
6
Gravitational waves from neutron stars and asteroseismology.来自中子星的引力波与星震学。
Philos Trans A Math Phys Eng Sci. 2018 May 28;376(2120). doi: 10.1098/rsta.2017.0285.
7
Proceedings of the International Workshop on Current Challenges in Liquid and Glass Science, (The Cosener's House, Abingdon 10-12 January 2007).《液体与玻璃科学当前挑战国际研讨会论文集》(2007年1月10日至12日于阿宾登科森纳之家)
J Phys Condens Matter. 2007 Oct 17;19(41):410301. doi: 10.1088/0953-8984/19/41/410301.
8
Probing high-momentum protons and neutrons in neutron-rich nuclei.探测富含中子核中的高动量质子和中子。
Nature. 2018 Aug;560(7720):617-621. doi: 10.1038/s41586-018-0400-z. Epub 2018 Aug 13.
9
Is a Trineutron Resonance Lower in Energy than a Tetraneutron Resonance?三中子共振的能量是否低于四中子共振?
Phys Rev Lett. 2017 Jun 9;118(23):232501. doi: 10.1103/PhysRevLett.118.232501. Epub 2017 Jun 8.
10
Surface emission from neutron stars and implications for the physics of their interiors.中子星的表面辐射及其对内部物理的影响。
Rep Prog Phys. 2013 Jan;76(1):016901. doi: 10.1088/0034-4885/76/1/016901. Epub 2012 Dec 12.

引用本文的文献

1
First observation of O.O 的首次观察。
Nature. 2023 Aug;620(7976):965-970. doi: 10.1038/s41586-023-06352-6. Epub 2023 Aug 30.