• 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

相似文献

1
Study of Total, Absorption, and He and H Production Cross Sections in He-proton Collisions.氦-质子碰撞中总截面、吸收截面以及氦和氢产生截面的研究。
Nucl Instrum Methods Phys Res B. 2021 Sep 1;502:136-141. doi: 10.1016/j.nimb.2021.06.013. Epub 2021 Jul 5.
2
Isotopic production cross sections in proton-16O and proton-12C interactions for energies from 10 MeV/u to 100 GeV/u.能量范围从10 MeV/u至100 GeV/u时,质子与16O以及质子与12C相互作用中的同位素产生截面。
Nucl Instrum Methods Phys Res B. 2023 Jan 1;534:26-34. doi: 10.1016/j.nimb.2022.11.005. Epub 2022 Nov 16.
3
Double-differential light-ion production cross sections.双微分轻离子产生截面。
Radiat Prot Dosimetry. 2004;110(1-4):57-60. doi: 10.1093/rpd/nch153.
4
Abrasion-ablation model for neutron production in heavy ion collisions.重离子碰撞中中子产生的擦除-烧蚀模型。
Nucl Phys A. 1997 Jun 16;619(1-2):202-12. doi: 10.1016/s0375-9474(97)00130-9.
5
Forward production of protons in relativistic 12C-nucleus collisions.相对论性碳 - 12原子核碰撞中质子的前向产生。
J Phys G Nucl Part Phys. 1994 Nov;20(11):1803-15. doi: 10.1088/0954-3899/20/11/009.
6
Light ion components of the galactic cosmic rays: nuclear interactions and transport theory.银河宇宙射线的轻离子成分:核相互作用与输运理论。
Adv Space Res. 1996;17(2):77-86. doi: 10.1016/0273-1177(95)00515-g.
7
Extension of PENELOPE to protons: simulation of nuclear reactions and benchmark with Geant4.将 PENELOPE 扩展到质子:核反应模拟及与 Geant4 的基准测试。
Med Phys. 2013 Nov;40(11):111705. doi: 10.1118/1.4823469.
8
Theoretical model of HZE particle fragmentation by hydrogen targets.氢靶对高电荷态重离子(HZE)粒子碎片化的理论模型。
Adv Space Res. 1996;17(2):109-12. doi: 10.1016/0273-1177(95)00519-k.
9
Microscopic optical model calculations of 4He, 12C-nucleus absorption cross sections.4He、12C核吸收截面的微观光学模型计算
J Phys G Nucl Part Phys. 1996 Mar;22(3):387-96. doi: 10.1088/0954-3899/22/3/012.
10
Cosmic ray radiation effects caused by proton-induced fragmentation.质子诱导碎裂引起的宇宙射线辐射效应。
Radiat Meas. 1997;28(1-6):537-42. doi: 10.1016/s1350-4487(97)00135-2.

引用本文的文献

1
Isotopic production cross sections in proton-16O and proton-12C interactions for energies from 10 MeV/u to 100 GeV/u.能量范围从10 MeV/u至100 GeV/u时,质子与16O以及质子与12C相互作用中的同位素产生截面。
Nucl Instrum Methods Phys Res B. 2023 Jan 1;534:26-34. doi: 10.1016/j.nimb.2022.11.005. Epub 2022 Nov 16.

本文引用的文献

1
Properties of Cosmic Helium Isotopes Measured by the Alpha Magnetic Spectrometer.《阿尔法磁谱仪测量的宇宙氦同位素性质》
Phys Rev Lett. 2019 Nov 1;123(18):181102. doi: 10.1103/PhysRevLett.123.181102.
2
Predictions of space radiation fatality risk for exploration missions.探索任务的空间辐射致死风险预测。
Life Sci Space Res (Amst). 2017 May;13:1-11. doi: 10.1016/j.lssr.2017.01.005. Epub 2017 Feb 1.
3
PAMELA measurements of cosmic-ray proton and helium spectra.PAMELA 对宇宙射线质子和氦谱的测量。
Science. 2011 Apr 1;332(6025):69-72. doi: 10.1126/science.1199172. Epub 2011 Mar 3.
4
Medium modified two-body scattering amplitude from proton-nucleus total cross-sections.由质子-原子核总截面得出的介质修正两体散射振幅。
Nucl Instrum Methods Phys Res B. 2001 Feb;173(4):391-6. doi: 10.1016/s0168-583x(00)00414-6.
5
Optical model methods of predicting nuclide production from spallation reactions.预测散裂反应中核素产生的光学模型方法。
Phys Rev C Nucl Phys. 1998 Feb;57(2):982-5. doi: 10.1103/physrevc.57.982.
6
Abrasion-ablation model for neutron production in heavy ion collisions.重离子碰撞中中子产生的擦除-烧蚀模型。
Nucl Phys A. 1997 Jun 16;619(1-2):202-12. doi: 10.1016/s0375-9474(97)00130-9.
7
Light ion components of the galactic cosmic rays: nuclear interactions and transport theory.银河宇宙射线的轻离子成分:核相互作用与输运理论。
Adv Space Res. 1996;17(2):77-86. doi: 10.1016/0273-1177(95)00515-g.
8
A simplified optical model description of heavy ion fragmentation.重离子碎裂的简化光学模型描述。
Can J Phys. 1985;63:135-8. doi: 10.1139/p85-021.
9
Correlations in alpha-alpha scattering and semi-classical optical models.α-α散射与半经典光学模型中的相关性。
Phys Lett B. 1989 Jun 8;223(2):127-32. doi: 10.1016/0370-2693(89)90226-8.
10
Production of 3H at large momentum in alpha-12C collisions at 2A GeV.在2A GeV的α粒子与碳 - 12碰撞中产生大动量的³H。
Phys Lett B. 1992 May 21;282(1-2):1-6. doi: 10.1016/0370-2693(92)90469-k.

氦-质子碰撞中总截面、吸收截面以及氦和氢产生截面的研究。

Study of Total, Absorption, and He and H Production Cross Sections in He-proton Collisions.

作者信息

Yan Congchong, Saganti Premkumar B, Cucinotta Francis A

机构信息

State Key Laboratory of Radiation Medicine and Protection, Collaborative Innovation Center of Radiation Medicine of Jiangsu Higher Education Institutions, School of Radiation Medicine and Protection, Soochow University, Suzhou, China.

Physics Department, Prairie View A&M University, Prairie View TX, United States of America.

出版信息

Nucl Instrum Methods Phys Res B. 2021 Sep 1;502:136-141. doi: 10.1016/j.nimb.2021.06.013. Epub 2021 Jul 5.

DOI:10.1016/j.nimb.2021.06.013
PMID:34898771
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC8654085/
Abstract

Light ion breakup cross sections are important for studies of cosmic ray interactions in the inter-stellar medium or radiation protection considerations of energy deposition in shielding and tissues. Abrasion cross sections for heavy ion reactions have been modeled using the Glauber model in the large mass limit or Eikonal form of the optical potential model. Here we formulate an abrasion model for He fragmentation on protons using the Glauber model avoiding the large mass limit and include a model for final state interactions. Calculations of energy dependent total, absorption, elastic and breakup cross sections for He into He or H with proton targets are shown to be in good agreement with experiments for energies from 100 to 100,000 MeV/u. The Glauber model for light nuclei with and without a large mass limit approximation is shown to be in fair agreement above 300 MeV/u, however important differences occur at lower energies.

摘要

轻离子破裂截面对于研究星际介质中的宇宙射线相互作用或屏蔽和组织中能量沉积的辐射防护考量而言至关重要。重离子反应的磨蚀截面已在大质量极限下使用格劳伯模型或光学势模型的程函形式进行了建模。在此,我们使用格劳伯模型为质子上的氦碎裂制定了一个磨蚀模型,避免了大质量极限,并纳入了一个末态相互作用模型。对于质子靶,氦与氦或氢相互作用时能量相关的总截面、吸收截面、弹性截面和破裂截面的计算结果表明,在100至100,000 MeV/u的能量范围内与实验结果吻合良好。有和没有大质量极限近似的轻核格劳伯模型在高于300 MeV/u时显示出相当一致的结果,然而在较低能量下会出现重要差异。