利用基于雅库茨克 EAS 阵列数据的μ介子相关法估算超高能宇宙射线的构成

IF 1.4 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY
A. V. Glushkov, L. T. Ksenofontov, K. G. Lebedev, A. V. Saburov
{"title":"利用基于雅库茨克 EAS 阵列数据的μ介子相关法估算超高能宇宙射线的构成","authors":"A. V. Glushkov,&nbsp;L. T. Ksenofontov,&nbsp;K. G. Lebedev,&nbsp;A. V. Saburov","doi":"10.1134/S002136402460188X","DOIUrl":null,"url":null,"abstract":"<p>In this article a new method is proposed for estimating the mass composition of cosmic rays in individual events with energies above <span>\\(1.25 \\times {{10}^{{19}}}\\)</span> eV. It is based on a joint analysis of experimental data and simulation results obtained using the QGSjet-II.04 model for muons with threshold energy <span>\\({{E}_{\\mu }} = 1.0 \\times \\cos \\theta \\)</span> GeV in air showers with zenith angles up to 60°. The data from ground-based and underground scintillation detectors of the Yakutsk EAS array were used. Separate groups of nuclei and other primary particles were found.</p>","PeriodicalId":604,"journal":{"name":"JETP Letters","volume":"120 6","pages":"396 - 403"},"PeriodicalIF":1.4000,"publicationDate":"2024-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Estimation of the Composition of Ultra-High Energy Cosmic Rays Using the Muon Correlation Method Based on Yakutsk EAS Array Data\",\"authors\":\"A. V. Glushkov,&nbsp;L. T. Ksenofontov,&nbsp;K. G. Lebedev,&nbsp;A. V. Saburov\",\"doi\":\"10.1134/S002136402460188X\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>In this article a new method is proposed for estimating the mass composition of cosmic rays in individual events with energies above <span>\\\\(1.25 \\\\times {{10}^{{19}}}\\\\)</span> eV. It is based on a joint analysis of experimental data and simulation results obtained using the QGSjet-II.04 model for muons with threshold energy <span>\\\\({{E}_{\\\\mu }} = 1.0 \\\\times \\\\cos \\\\theta \\\\)</span> GeV in air showers with zenith angles up to 60°. The data from ground-based and underground scintillation detectors of the Yakutsk EAS array were used. Separate groups of nuclei and other primary particles were found.</p>\",\"PeriodicalId\":604,\"journal\":{\"name\":\"JETP Letters\",\"volume\":\"120 6\",\"pages\":\"396 - 403\"},\"PeriodicalIF\":1.4000,\"publicationDate\":\"2024-11-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"JETP Letters\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://link.springer.com/article/10.1134/S002136402460188X\",\"RegionNum\":4,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q3\",\"JCRName\":\"PHYSICS, MULTIDISCIPLINARY\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"JETP Letters","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1134/S002136402460188X","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"PHYSICS, MULTIDISCIPLINARY","Score":null,"Total":0}
引用次数: 0

摘要

本文提出了一种新方法,用于估算能量超过 \(1.25 \times {{10}^{{19}}}\) eV 的单个事件中宇宙射线的质量组成。它基于对实验数据的联合分析,以及使用 QGSjet-II.04 模型对天顶角达到 60°的空气阵列中阈值能量为 \({{E}_{\mu }} = 1.0 \times \cos \theta \) GeV 的μ介子的模拟结果。使用的数据来自雅库茨克 EAS 阵列的地面和地下闪烁探测器。发现了独立的原子核和其他原生粒子群。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Estimation of the Composition of Ultra-High Energy Cosmic Rays Using the Muon Correlation Method Based on Yakutsk EAS Array Data

Estimation of the Composition of Ultra-High Energy Cosmic Rays Using the Muon Correlation Method Based on Yakutsk EAS Array Data

In this article a new method is proposed for estimating the mass composition of cosmic rays in individual events with energies above \(1.25 \times {{10}^{{19}}}\) eV. It is based on a joint analysis of experimental data and simulation results obtained using the QGSjet-II.04 model for muons with threshold energy \({{E}_{\mu }} = 1.0 \times \cos \theta \) GeV in air showers with zenith angles up to 60°. The data from ground-based and underground scintillation detectors of the Yakutsk EAS array were used. Separate groups of nuclei and other primary particles were found.

求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
JETP Letters
JETP Letters 物理-物理:综合
CiteScore
2.40
自引率
30.80%
发文量
164
审稿时长
3-6 weeks
期刊介绍: All topics of experimental and theoretical physics including gravitation, field theory, elementary particles and nuclei, plasma, nonlinear phenomena, condensed matter, superconductivity, superfluidity, lasers, and surfaces.
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信