Limits to gauge coupling in the dark sector of super-heavy dark matter particles from the Pierre Auger Observatory data

Olivier Deligny
{"title":"Limits to gauge coupling in the dark sector of super-heavy dark matter particles from the Pierre Auger Observatory data","authors":"Olivier Deligny","doi":"10.21468/scipostphysproc.13.013","DOIUrl":null,"url":null,"abstract":"Assuming that the energy density of super-heavy particles matches that of dark matter observed today, tight constraints on the couplings governing the decay process are presented as a function of the particle mass. These constraints are obtained from the lack of signatures that would be suggestive of decaying super-heavy X <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mi>X</mml:mi></mml:math> particles in the data of the Pierre Auger Observatory. In particular, instanton-induced decay processes allow us to derive a bound on the reduced coupling constant of gauge interactions in the dark sector: \\alpha_X \\lesssim 0.09 <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mrow><mml:msub><mml:mi>α</mml:mi><mml:mi>X</mml:mi></mml:msub><mml:mo>≲</mml:mo><mml:mn>0.09</mml:mn></mml:mrow></mml:math> , for 10^{9} \\lesssim M_X/\\mathrm{GeV} &amp;lt; 10^{19} <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mrow><mml:msup><mml:mn>10</mml:mn><mml:mn>9</mml:mn></mml:msup><mml:mo>≲</mml:mo><mml:msub><mml:mi>M</mml:mi><mml:mi>X</mml:mi></mml:msub><mml:mi>/</mml:mi><mml:mstyle mathvariant=\"normal\"><mml:mi>G</mml:mi><mml:mi>e</mml:mi><mml:mi>V</mml:mi></mml:mstyle><mml:mo><</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mn>19</mml:mn></mml:msup></mml:mrow></mml:math> . Cosmological aspects for super-heavy dark matter production during the reheating epoch are discussed.","PeriodicalId":355998,"journal":{"name":"SciPost Physics Proceedings","volume":"64 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2023-09-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"SciPost Physics Proceedings","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.21468/scipostphysproc.13.013","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 1

Abstract

Assuming that the energy density of super-heavy particles matches that of dark matter observed today, tight constraints on the couplings governing the decay process are presented as a function of the particle mass. These constraints are obtained from the lack of signatures that would be suggestive of decaying super-heavy X X particles in the data of the Pierre Auger Observatory. In particular, instanton-induced decay processes allow us to derive a bound on the reduced coupling constant of gauge interactions in the dark sector: \alpha_X \lesssim 0.09 αX0.09 , for 10^{9} \lesssim M_X/\mathrm{GeV} &lt; 10^{19} 109MX/GeV<1019 . Cosmological aspects for super-heavy dark matter production during the reheating epoch are discussed.
皮埃尔·奥格天文台数据对超重暗物质粒子暗区测量耦合的限制
假设超重粒子的能量密度与今天观测到的暗物质的能量密度相匹配,那么控制衰变过程的耦合的严格约束将作为粒子质量的函数呈现出来。这些限制是由于缺乏在皮埃尔·奥格天文台的数据中暗示衰变的超重X粒子的特征而得到的。特别是,瞬态诱导的衰变过程允许我们推导出暗扇区中规范相互作用的简化耦合常数的界:\alpha _X \lesssim 0.09 αX > 0.09,对于10^{9}\lesssim M_X/ \mathrm{GeV} &lt;10^{19} 109 > MX/GeV&lt;1019。讨论了重热时期超重暗物质产生的宇宙学问题。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 求助全文
来源期刊
自引率
0.00%
发文量
0
×
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