伽马射线,中微子和宇宙射线来自疏散星团的密集区域

W. Bednarek, J. Pabich, T. Sobczak
{"title":"伽马射线,中微子和宇宙射线来自疏散星团的密集区域","authors":"W. Bednarek,&nbsp;J. Pabich,&nbsp;T. Sobczak","doi":"10.1016/j.nuclphysbps.2014.10.013","DOIUrl":null,"url":null,"abstract":"<div><p>We analyse the high energy processes, occurring within open clusters containing massive binary systems, which turn to the production of high energy <em>γ</em>-rays and neutrinos. Nuclei, accelerated within the binary systems, inject protons and neutrons as a result of their fragmentation in collisions with stellar radiation and matter of the winds. We calculate the radiation produced by these protons and neutrons during their interaction with the matter of the stellar wind and the open cluster. The detectability of <em>γ</em>-ray emission and neutrino emission by the present and future Cherenkov telescopes and the neutrino telescopes is discussed.</p></div>","PeriodicalId":93343,"journal":{"name":"Nuclear physics. B, Proceedings, supplements","volume":"256 ","pages":"Pages 107-116"},"PeriodicalIF":0.0000,"publicationDate":"2014-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/j.nuclphysbps.2014.10.013","citationCount":"3","resultStr":"{\"title\":\"Gamma-rays, neutrinos and cosmic rays from dense regions in open clusters\",\"authors\":\"W. Bednarek,&nbsp;J. Pabich,&nbsp;T. Sobczak\",\"doi\":\"10.1016/j.nuclphysbps.2014.10.013\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>We analyse the high energy processes, occurring within open clusters containing massive binary systems, which turn to the production of high energy <em>γ</em>-rays and neutrinos. Nuclei, accelerated within the binary systems, inject protons and neutrons as a result of their fragmentation in collisions with stellar radiation and matter of the winds. We calculate the radiation produced by these protons and neutrons during their interaction with the matter of the stellar wind and the open cluster. The detectability of <em>γ</em>-ray emission and neutrino emission by the present and future Cherenkov telescopes and the neutrino telescopes is discussed.</p></div>\",\"PeriodicalId\":93343,\"journal\":{\"name\":\"Nuclear physics. B, Proceedings, supplements\",\"volume\":\"256 \",\"pages\":\"Pages 107-116\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2014-11-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://sci-hub-pdf.com/10.1016/j.nuclphysbps.2014.10.013\",\"citationCount\":\"3\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Nuclear physics. B, Proceedings, supplements\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S0920563214002072\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Nuclear physics. B, Proceedings, supplements","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0920563214002072","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 3

摘要

我们分析了发生在包含大质量双星系统的疏散星团内的高能过程,这些过程转向产生高能γ射线和中微子。在双星系统中加速的原子核在与恒星辐射和风中的物质碰撞时破碎,从而注入质子和中子。我们计算了这些质子和中子在与恒星风和疏散星团的物质相互作用时产生的辐射。讨论了现在和将来的切伦科夫望远镜和中微子望远镜对γ射线发射和中微子发射的可探测性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
Gamma-rays, neutrinos and cosmic rays from dense regions in open clusters

We analyse the high energy processes, occurring within open clusters containing massive binary systems, which turn to the production of high energy γ-rays and neutrinos. Nuclei, accelerated within the binary systems, inject protons and neutrons as a result of their fragmentation in collisions with stellar radiation and matter of the winds. We calculate the radiation produced by these protons and neutrons during their interaction with the matter of the stellar wind and the open cluster. The detectability of γ-ray emission and neutrino emission by the present and future Cherenkov telescopes and the neutrino telescopes is discussed.

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
自引率
0.00%
发文量
0
期刊最新文献
Contents Editorial Board Author index Hybrid Simulations of Particle Acceleration at Shocks Using optical lines to study particle acceleration at supernova remnants
×
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
现在去查看 取消
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术
文献互助 智能选刊 最新文献 互助须知 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 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1